Author: "Astronomy and Astrophysics Research Group" - Searchworks@Jio Institute Digital Library Search Results

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141 results on '"Astronomy and Astrophysics Research Group"'

1. In situ, broadband measurement of the radio frequency attenuation length at Summit Station, Greenland

Author: J. A. Aguilar, P. Allison, J. J. Beatty, D. Besson, A. Bishop, O. Botner, S. Bouma, S. Buitink, M. Cataldo, B. A. Clark, Z. Curtis-Ginsberg, A. Connolly, P. Dasgupta, S. de Kockere, K. D. de Vries, C. Deaconu, M. A. DuVernois, C. Glaser, A. Hallgren, S. Hallmann, J. C. Hanson, B. Hendricks, C. Hornhuber, K. Hughes, A. Karle, J. L. Kelley, I. Kravchenko, R. Krebs, R. Lahmann, U. Latif, J. Mammo, Z. S. Meyers, K. Michaels, K. Mulrey, A. Nelles, A. Novikov, A. Nozdrina, E. Oberla, B. Oeyen, Y. Pan, H. Pandya, I. Plaisier, N. Punsuebsay, L. Pyras, D. Ryckbosch, O. Scholten, D. Seckel, M. F. H. Seikh, D. Smith, D. Southall, J. Torres, S. Toscano, D. Tosi, D. J. Van Den Broeck, N. van Eijndhoven, A. G. Vieregg, C. Welling, D. R. Williams, S. Wissel, R. Young, A. Zink, Physics, Astronomy and Astrophysics Research Group, Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, and Astronomy
Subjects: electron, Astronomy, ice thickness measurements, Astrophysics::High Energy Astrophysical Phenomena, ice, FOS: Physical sciences, ZONE, High Energy Physics - Experiment, ENERGY, High Energy Physics - Experiment (hep-ex), Astronomi, astrofysik och kosmologi, Ground-penetrating radar, neutrino: energy, ddc:550, Astronomy, Astrophysics and Cosmology, CORE, ROSS ICE SHELF, Instrumentation and Methods for Astrophysics (astro-ph.IM), Earth-Surface Processes, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, radio wave, hep-ex, ice physics, PERFORMANCE, length [attenuation], neutrino: UHE, UHE [neutrino], electric field, ANTARCTICA, observatory, Physics and Astronomy, attenuation: length, energy [neutrino], radio-echo sounding, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, astro-ph.IM
Abstract: Journal of glaciology 40, 1 - 9 (2022). doi:10.1017/jog.2022.40, Over the last 25 years, radiowave detection of neutrino-generated signals, using cold polar ice as the neutrino target, has emerged as perhaps the most promising technique for detection of extragalactic ultra-high energy neutrinos (corresponding to neutrino energies in excess of 0.01 Joules, or $10^{17}$ electron volts). During the summer of 2021 and in tandem with the initial deployment of the Radio Neutrino Observatory in Greenland (RNO-G), we conducted radioglaciological measurements at Summit Station, Greenland to refine our understanding of the ice target. We report the result of one such measurement, the radio-frequency electric field attenuation length $L_\alpha$. We find an approximately linear dependence of $L_\alpha$ on frequency with the best fit of the average field attenuation for the upper 1500 m of ice: $\langle L_\alpha \rangle = \big( (1154 \pm 121) - (0.81 \pm 0.14) (\nu/$MHz$)\big)$ m for frequencies $\nu \in [145 - 350]$ MHz., Published by Soc., Cambridge
Published: 2022
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2. CO line observations of OH/IR stars in the inner Galactic Bulge

Author: Olofsson, H., Khouri, T., Sargent, B. A., Winnberg, A., Blommaert, J. A. D. L., Groenewegen, M. A. T., Muller, S., Kastner, J. H., Meixner, M., Otsuka, M., Patel, N., Ryde, N., Srinivasan, S., Physics, and Astronomy and Astrophysics Research Group
Subjects: astro-ph.SR, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), astro-ph.GA, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Solar and Stellar Astrophysics (astro-ph.SR)
Abstract: 12CO and 13CO lines, as well as a mm-wave continuum, have been observed for a sample of 22 OH/IR stars in directions within 2 degrees of the Galactic Centre. Photometry data have been gathered from the literature to construct SEDs and to determine pulsational variability. Radiative transfer models have been used to interpret the data. All stars in the sample were detected in at least one CO line, and 8 objects were detected in 324 GHz continuum. Based on luminosity criteria, the sample is divided into 17 objects that most likely lie within the inner Galactic Bulge, and 5 objects that are most likely foreground objects. The median luminosity of the inner-Galactic-Bulge objects, 5600 Lsun, corresponds to an initial mass in the range 1.2-1.6 Msun, indicating that these OH/IR stars descend from solar-type stars. The objects in this sub-sample are further divided into two classes based on their SED characteristics: 11 objects have SEDs that are well matched by models invoking dust envelopes extending from a few stellar radii and outwards, while 6 objects are better modelled as having detached dust envelopes with inner radii in the range 200-600 au and warmer central stars. The former objects have periodic variability, while the latter objects are predominantly non-periodic. The median gas-mass-loss rate, gas terminal expansion velocity, gas-to-dust mass ratio, and circumstellar 12CO/13CO abundance ratio have been estimated to be 2x10{-5} Msun/yr, 18 km/s, 200 (excluding the sources with detached dust envelopes, which show markedly lower gas-to-dust ratios), and 5, respectively, for the inner-Galactic-Bulge objects. The inner-Galactic-Bulge OH/IR stars studied here constitute an excellent sample of equidistant objects for the purpose of understanding the evolution of the mass-loss-rate characteristics at the tip of the AGB., 32 pages, 17 figures
Published: 2022
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3. Determining Atmospheric Electric Fields using MGMR3D

Author: T. N. G. Trinh, O. Scholten, S. Buitink, K. D. de Vries, P. Mitra, T. Phong Nguyen, D. T. Si, Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, and Astronomy
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Cosmic-ray particles impinging on the atmosphere induce high-energy particle cascades in air, an Extensive Air Shower (EAS), emitting coherent radio emission. This emission is affected by the presence of strong electric fields during thunderstorm conditions. To reconstruct the atmospheric electric field from the measured radio footprint of the EAS we use an analytic model for the calculation of the radio emission, MGMR3D. In this work we make an extensive comparison between the results of a microscopic model for radio emission, CoREAS, to obtain an improved parametrization for MGMR3D in the presence of atmospheric electric fields, as well as confidence intervals. The approach to extract the electric field structure is applied successfully to an event with a complicated radio footprint measured by LOFAR during thunderstorm conditions. This shows that, with the improved parametrization, MGMR3D can be used to extract the structure of the atmospheric electric field., The paper is accepted for publication in Physical Review D
Published: 2022

4. Interferometric imaging of intensely radiating negative leaders

Author: O. Scholten, B. M. Hare, J. Dwyer, N. Liu, C. Sterpka, I. Kolmašová, O. Santolík, R. Lán, L. Uhlíř, S. Buitink, T. Huege, A. Nelles, S. ter Veen, Astronomy, Physics, and Astronomy and Astrophysics Research Group
Subjects: Physics - Atmospheric and Oceanic Physics, Astronomy, Atmospheric and Oceanic Physics (physics.ao-ph), FOS: Physical sciences, physics.ao-ph, ddc:530, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), astro-ph.IM
Abstract: Physical review / D 105(6), 062007 (2022). doi:10.1103/PhysRevD.105.062007, The common phenomenon of lightning still harbors many secrets and only recently a new propagation mode was observed for negative leaders. While propagating in this “intensely radiating negative leader” (IRNL) mode a negative leader emits 100 times more very-high frequency (VHF) and broadband radiation than a more normal negative leader. We have reported that this mode occurs soon after initiation of all lightning flashes we have mapped as well as sometimes long thereafter. Because of the profuse emission of VHF the leader structure is very difficult to image. In this work we report on measurements made with the LOFAR radio telescope, an instrument primarily built for radio-astronomy observations. For this reason, as part of the present work, we have refined our time resolved interferometric 3-dimensional (TRI-D) imaging to take into account the antenna function. The images from the TRI-D imager show that during an IRNL there is an ionization front with a diameter in excess of 500 m where strong corona bursts occur. This is very different from what is seen for a normal negative leader where the corona bursts happen at the tip, an area of typically 10 m in diameter. The observed massive ionization wave supports the idea that this mode is indicative of a dense charge pocket., Published by Inst., Melville, NY
Published: 2022
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5. Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

Author: The Pierre Auger Collaboration, Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Cheminant, K. Almeida, Almela, A., Alvarez-Muñiz, J., Batista, R. Alves, Yebra, J. Ammerman, Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ferreira, P. R. Araújo, Arnone, E., Velázquez, J. C. Arteaga, Asorey, H., Assis, P., Avila, G., Avocone, E., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Bellido, J. A., Berat, C., Bertaina, M. E., Bhatta, G., Biermann, P. L., Binet, V., Bismark, K., Bister, T., Biteau, J., Blazek, J., Bleve, C., Blümer, J., Boháčová, M., Boncioli, D., Bonifazi, C., Arbeletche, L. Bonneau, Borodai, N., Botti, A. M., Brack, J., Bretz, T., Orchera, P. G. Brichetto, Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Büsken, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobos, Colalillo, R., Coleman, A., Coluccia, M. R., Conceição, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Santos, D. Correia dos, Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jesús, J., de Jong, S. J., Neto, J. R. T. de Mello, De Mitri, I., de Oliveira, J., Franco, D. de Oliveira, de Palma, F., de Souza, V., De Vito, E., Del Popolo, A., del Río, M., Deligny, O., Deval, L., di Matteo, A., Dobre, M., Dobrigkeit, C., D'Olivo, J. C., Mendes, L. M. Domingues, Anjos, R. C. dos, Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipčič, A., Fitoussi, T., Fodran, T., Fujii, T., Fuster, A., Galea, C., Galelli, C., García, B., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, Gongora, J. P., González, J. M., González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., Kääpä, A., Kampert, K. H., Keilhauer, B., Khakurdikar, A., Covilakam, V. V. Kizakke, Klages, H. O., Kleifges, M., Kleinfeller, J., Knapp, F., Kunka, N., Lago, B. L., Langner, N., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Presti, D. Lo, Lopes, L., López, R., Lu, L., Luce, Q., Lundquist, J. P., Payeras, A. Machado, Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariani, F. M., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Martinelli, S., Bravo, O. Martínez, Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mayotte, S., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morejon, L., Morello, C., Mostafá, M., Müller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Nicora, G., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Norwood, I., Nosek, D., Novotny, V., Nožka, L., Nucita, A, Núñez, L. A., Oliveira, C., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pawlowsky, J., Pech, M., Pękala, J., Pelayo, R., Peña-Rodriguez, J., Martins, E. E. Pereira, Armand, J. Perez, Bertolli, C. Pérez, Perrone, L., Petrera, S., Petrucci, C., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., de Carvalho, W. Rodrigues, Rojo, J. Rodriguez, Roncoroni, M. J., Rossoni, S., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saftoiu, A., Saharan, M., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. Sanabria, Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sato, R., Savina, P., Schäfer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schlüter, F., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schröder, F. G., Schulte, J., Schulz, T., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smau, R., Šmída, R., Sommers, P., Soriano, J. F., Squartini, R., Stadelmaier, M., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Straub, M., Streich, A., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Szadkowski, Z., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Peixoto, C. J. Todero, Tomé, B., Torrès, Z., Travaini, A., Travnicek, P., Trimarelli, C., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Galicia, J. F. Valdés, Valore, L., Varela, E., Vásquez-Ramírez, A., Veberič, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weindl, A., Wiencke, L., Wilczyński, H., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Abreu, P, Aglietta, M, Albury, Jm, Allekotte, I, Cheminant, Ka, Almela, A, Alvarez-Muniz, J, Batista, Ra, Yebra, Ja, Anastasi, Ga, Anchordoqui, L, Andrada, B, Andringa, S, Aramo, C, Ferreira, Pra, Arnone, E, Velazquez, Jca, Asorey, H, Assis, P, Avila, G, Avocone, E, Badescu, Am, Bakalova, A, Balaceanu, A, Barbato, F, Bellido, Ja, Berat, C, Bertaina, Me, Bhatta, G, Biermann, Pl, Binet, V, Bismark, K, Bister, T, Biteau, J, Blazek, J, Bleve, C, Blumer, J, Bohacova, M, Boncioli, D, Bonifazi, C, Arbeletche, Lb, Borodai, N, Botti, Am, Brack, J, Bretz, T, Orchera, Pgb, Briechle, Fl, Buchholz, P, Bueno, A, Buitink, S, Buscemi, M, Busken, M, Caballero-Mora, K, Caccianiga, L, Canfora, F, Caracas, I, Caruso, R, Castellina, A, Catalani, F, Cataldi, G, Cazon, L, Cerda, M, Chinellato, Ja, Chudoba, J, Chytka, L, Clay, Rw, Cerutti, Acc, Colalillo, R, Coleman, A, Coluccia, Mr, Conceicao, R, Condorelli, A, Consolati, G, Contreras, F, Convenga, F, dos Santos, Dc, Covault, Ce, Dasso, S, Daumiller, K, Dawson, Br, Day, Ja, de Almeida, Rm, de Jesus, J, de Jong, Sj, Neto, Jrtd, De Mitri, I, de Oliveira, J, Franco, Dd, de Palma, F, de Souza, V, De Vito, E, Del Popolo, A, del Rio, M, Deligny, O, Deval, L, di Matteo, A, Dobre, M, Dobrigkeit, C, D'Olivo, Jc, Mendes, Lmd, dos Anjos, Rc, Dova, Mt, Ebr, J, Engel, R, Epicoco, I, Erdmann, M, Escobar, Co, Etchegoyen, A, Falcke, H, Farmer, J, Farrar, G, Fauth, Ac, Fazzini, N, Feldbusch, F, Fenu, F, Fick, B, Figueira, Jm, Fitoussi, T, Fodran, T, Fujii, T, Fuster, A, Galea, C, Galelli, C, Garcia, B, Gemmeke, H, Gesualdi, F, Gherghel-Lascu, A, Ghia, Pl, Giaccari, U, Giammarchi, M, Glombitza, J, Gobbi, F, Gollan, F, Golup, G, Berisso, Mg, Vitale, Pfg, Gongora, Jp, Gonzalez, Jm, Gonzalez, N, Goos, I, Gora, D, Gorgi, A, Gottowik, M, Grubb, Td, Guarino, F, Guedes, Gp, Guido, E, Hahn, S, Hamal, P, Hampel, Mr, Hansen, P, Harari, D, Harvey, Vm, Haungs, A, Hebbeker, T, Heck, D, Hill, Gc, Hojvat, C, Horandel, Jr, Horvath, P, Hrabovsky, M, Huege, T, Insolia, A, Isar, Pg, Janecek, P, Johnsen, Ja, Jurysek, J, Kaapa, A, Kampert, Kh, Keilhauer, B, Khakurdikar, A, Covilakam, Vvk, Klages, Ho, Kleifges, M, Kleinfeller, J, Knapp, F, Kunka, N, Lago, Bl, Langner, N, de Oliveira, Mal, Lenok, V, Letessier-Selvon, A, Lhenry-Yvon, I, Lo Presti, D, Lopes, L, Lopez, R, Lu, L, Luce, Q, Lundquist, Jp, Payeras, Am, Mancarella, G, Mandat, D, Manning, Bc, Manshanden, J, Mantsch, P, Marafico, S, Mariani, Fm, Mariazzi, Ag, Maris, Ic, Marsella, G, Martello, D, Martinelli, S, Bravo, Om, Mastrodicasa, M, Mathes, Hj, Matthews, J, Matthiae, G, Mayotte, E, Mayotte, S, Mazur, Po, Medina-Tanco, G, Melo, D, Menshikov, A, Michal, S, Micheletti, Mi, Miramonti, L, Mollerach, S, Montanet, F, Morejon, L, Morello, C, Mostafa, M, Muller, Al, Muller, Ma, Mulrey, K, Mussa, R, Muzio, M, Namasaka, Wm, Nasr-Esfahani, A, Nellen, L, Nicora, G, Niculescu-Oglinzanu, M, Niechciol, M, Nitz, D, Norwood, I, Nosek, D, Novotny, V, Nozka, L, Nucita, A, Nunez, La, Oliveira, C, Palatka, M, Pallotta, J, Papenbreer, P, Parente, G, Parra, A, Pawlowsky, J, Pech, M, Pekala, J, Pelayo, R, Pena-Rodriguez, J, Martins, Eep, Armand, Jp, Bertolli, Cp, Perrone, L, Petrera, S, Petrucci, C, Pierog, T, Pimenta, M, Pirronello, V, Platino, M, Pont, B, Pothast, M, Privitera, P, Prouza, M, Puyleart, A, Querchfeld, S, Rautenberg, J, Ravignani, D, Reininghaus, M, Ridky, J, Riehn, F, Risse, M, Rizi, V, de Carvalho, Wr, Rojo, Jr, Roncoroni, Mj, Rossoni, S, Roth, M, Roulet, E, Rovero, Ac, Ruehl, P, Saftoiu, A, Saharan, M, Salamida, F, Salazar, H, Salina, G, Gomez, Jd, Sanchez, F, Santos, Em, Santos, E, Sarazin, F, Sarmento, R, Sato, R, Savina, P, Schafer, Cm, Scherini, V, Schieler, H, Schimassek, M, Schimp, M, Schluter, F, Schmidt, D, Scholten, O, Schoorlemmer, H, Schovanek, P, Schroder, Fg, Schulte, J, Schulz, T, Sciutto, Sj, Scornavacche, M, Segreto, A, Sehgal, S, Shellard, Rc, Sigl, G, Silli, G, Sima, O, Smau, R, Smida, R, Sommers, P, Soriano, Jf, Squartini, R, Stadelmaier, M, Stanca, D, Stanic, S, Stasielak, J, Stassi, P, Straub, M, Streich, A, Suarez-Duran, M, Sudholz, T, Suomijarvi, T, Supanitsky, Ad, Szadkowski, Z, Tapia, A, Taricco, C, Timmermans, C, Tkachenko, O, Tobiska, P, Peixoto, Cjt, Tome, B, Torres, Z, Travaini, A, Travnicek, P, Trimarelli, C, Tueros, M, Ulrich, R, Unger, M, Vaclavek, L, Vacula, M, Galicia, Jfv, Valore, L, Varela, E, Vasquez-Ramirez, A, Veberic, D, Ventura, C, Quispe, Idv, Verzi, V, Vicha, J, Vink, J, Vorobiov, S, Wahlberg, H, Watanabe, C, Watson, Aa, Weindl, A, Wiencke, L, Wilczynski, H, Wittkowski, D, Wundheiler, B, Yushkov, A, Zapparrata, O, Zas, E, Zavrtanik, D, Zavrtanik, M, Zehrer, L, Physics, and Astronomy and Astrophysics Research Group
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astronomy, Astrophysics::High Energy Astrophysical Phenomena, cosmic radiation: energy, UHE [cosmic radiation], FOS: Physical sciences, anisotropy, energy [cosmic radiation], ddc:530, High Energy Physics, cosmic radiation: UHE, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), angular correlation, Physics, OBSERVATÓRIOS, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Auger, flux, observatory, Space and Planetary Science, Experimental High Energy Physics, astro-ph.CO, ddc:520, Astrophysics - High Energy Astrophysical Phenomena, Ultra-high-energy cosmic radiation, Cosmic ray astronomy, Clustering, Active galaxies, Starburst galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, experimental results
Abstract: A promising energy range to look for angular correlations between cosmic rays of extragalactic origin and their sources is at the highest energies, above a few tens of EeV (1 EeV ≡ 1018 eV). Despite the flux of these particles being extremely low, the area of ∼3000 km2 covered at the Pierre Auger Observatory, and the 17 yr data-taking period of the Phase 1 of its operations, have enabled us to measure the arrival directions of more than 2600 ultrahigh- energy cosmic rays above 32 EeV. We publish this data set, the largest available at such energies from an integrated exposure of 122,000 km2 sr yr, and search it for anisotropies over the 3.4π steradians covered with the Observatory. Evidence for a deviation in excess of isotropy at intermediate angular scales, with ∼15° Gaussian spread or ∼25° top-hat radius, is obtained at the 4σ significance level for cosmic-ray energies above ∼40 EeV., Argentina-Comision Nacional de Energia Atomica, ANPCyT, Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3, Ministry of Education, Youth & Sports - Czech Republic LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422, French National Research Agency (ANR) LABEX ANR-10-LABX-63 ANR-11-IDEX-0004-02, Consejo Nacional de Ciencia y Tecnologia (CONACyT) 167733, Netherlands Organization for Scientific Research (NWO) DIR/WK/2018/11, National Science Centre, Poland 2016/22/M/ST9/00198 2016/23/B/ST9/01635 2020/39/B/ST9/01398, Romania-Ministry of Research, Innovation and Digitization, CNCS/CCCDIUEFISCDI within PNCDI III PN19150201/16N/2019 PN1906010 TE128 PED289, Slovenian Research Agency - Slovenia P1-0031 P1-0385 I0-0033 N1-0111, Spanish Government FPA2017-85114-P PID2019-104676GB-C32, Xunta de Galicia, European Commission ED431C 2017/07, Junta de Andalucia Feder Funds SOMM17/6104/UGR P18-FR-4314, RENATA Red Nacional Tematica de Astroparticulas FPA2015-68783-REDT, Maria de Maeztu Unit of Excellence MDM-2016-0692, United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DE-FG02-99ER41107 DE-SC0011689, National Science Foundation (NSF) 0450696, Gobierno de la Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, Australian Research Council, Belgium -Fonds de la Recherche Scientifique (FNRS), FWO, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ), Fundacao de Apoio a Pesquisa do Distrito Federal (FAPDF), Financiadora de Inovacao e Pesquisa (Finep), Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio De Janeiro (FAPERJ), Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC), France-Centre de Calcul IN2P3/CNRS, France-Centre de Calcul IN2P3/CNRS Centre National de la Recherche Scientifique (CNRS) Departement Sciences de l'Univers (SDU-INSU/CNRS), Federal Ministry of Education & Research (BMBF) German Research Foundation (DFG) Finanzministerium Baden-Wurttemberg Helmholtz Alliance for Astroparticle Physics (HAP) Helmholtz Association Ministerium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg, Italy-Istituto Nazionale di Fisica Nucleare (INFN), Istituto Nazionale Astrofisica (INAF), Ministry of Education, Universities and Research (MIUR), CETEMPS Center of Excellence, Ministry of Foreign Affairs and International Cooperation (Italy), Universidad Nacional Autonoma de Mexico, Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPIIT), Netherlands-Ministry of Education, Culture and Science Netherlands Organization for Scientific Research (NWO), SURF Cooperative, Portuguese Foundation for Science and Technology, FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE), The Grainger Foundation x, Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, UNESCO
Published: 2022
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6. A Search for Photons with Energies Above 2 × 10$^{17}$ eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory

Author: Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Cheminant, K. A., Almela, A., Alvarez-Muñiz, J., Batista, R. A., Yebra, J. A., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ferreira, P. R. A., Arnone, E., Velázquez, J. C. A., Asorey, H., Assis, P., Avila, G., Avocone, E., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Bellido, J. A., Berat, C., Bertaina, M. E., Bhatta, G., Biermann, P. L., Binet, V., Bismark, K., Bister, T., Biteau, J., Blazek, J., Bleve, C., Blümer, J., Boháčová, M., Boncioli, D., Bonifazi, C., Arbeletche, L. B., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Orchera, P. G. B., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Büsken, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceição, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Dos Santos, D. C., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., De Almeida, R. M., De Jesús, J., De Jong, S. J., De Mello Neto, J. R. T., De Mitri, I., De Oliveira, J., De Oliveira Franco, D., De Palma, F., De Souza, V., De Vito, E., Del Popolo, A., Del Río, M., Deligny, O., Deval, L., Di Matteo, A., Dobre, M., Dobrigkeit, C., D’Olivo, J. C., Mendes, L. M. D., Dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipčič, A., Fitoussi, T., Fodran, T., Fujii, T., Fuster, A., Galea, C., Galelli, C., García, B., Vegas, A. L. G., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Berisso, M. G., Vitale, P. F. G., Gongora, J. P., González, J. M., González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., Kääpä, A., Kampert, K. H., Keilhauer, B., Khakurdikar, A., Covilakam, V. V. K., Klages, H. O., Kleifges, M., Kleinfeller, J., Knapp, F., Kunka, N., Lago, B. L., Langner, N., De Oliveira, M. A. L., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Presti, D. L., Lopes, L., López, R., Lu, L., Luce, Q., Lundquist, J. P., Payeras, A. M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariani, F. M., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Martinelli, S., Martínez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mayotte, S., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morejon, L., Morello, C., Mostafá, M., Müller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Nicora, G., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Norwood, I., Nosek, D., Novotny, V., Nožka, L., Nucita, A., Núñez, L. A., Oliveira, C., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pawlowsky, J., Pech, M., P ©kala, J., Pelayo, R., Peña-Rodriguez, J., Martins, E. E. P., Armand, J. P., Bertolli, C. P., Perrone, L., Petrera, S., Petrucci, C., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., De Carvalho, W. R., Rojo, J. R., Roncoroni, M. J., Rossoni, S., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saftoiu, A., Saharan, M., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. S., Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schäfer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schlüter, F., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovánek, P., Schröder, F. G., Schulte, J., Schulz, T., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smau, R., Šmída, R., Sommers, P., Soriano, J. F., Squartini, R., Stadelmaier, M., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Streich, A., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Szadkowski, Z., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Peixoto, C. J. T., Tomé, B., Torrès, Z., Travaini, A., Travnicek, P., Trimarelli, C., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Galicia, J. F. V., Valore, L., Varela, E., Vásquez-Ramírez, A., Veberič, D., Ventura, C., Quispe, I. D. V., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weindl, A., Wiencke, L., Wilczyński, H., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Pierre Auger Collaboration, High Energy Astrophys. & Astropart. Phys (API, FNWI), Astronomy and Astrophysics Research Group, Physics, Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Cheminant, K. A., Almela, A., Alvarez-Muniz, J., Batista, R. A., Yebra, J. A., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ferreira, P. R. A., Arnone, E., Velazquez, J. C. A., Asorey, H., Assis, P., Avila, G., Avocone, E., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Bellido, J. A., Berat, C., Bertaina, M. E., Bhatta, G., Biermann, P. L., Binet, V., Bismark, K., Bister, T., Biteau, J., Blazek, J., Bleve, C., Blumer, J., Bohacova, M., Boncioli, D., Bonifazi, C., Arbeletche, L. B., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Orchera, P. G. B., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Busken, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Dos Santos, D. C., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., De Almeida, R. M., De Jesus, J., De Jong, S. J., De Mello Neto, J. R. T., De Mitri, I., De Oliveira, J., De Oliveira Franco, D., De Palma, F., De Souza, V., De Vito, E., Del Popolo, A., Del Rio, M., Deligny, O., Deval, L., Di Matteo, A., Dobre, M., Dobrigkeit, C., D'Olivo, J. C., Mendes, L. M. D., Dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipcic, A., Fitoussi, T., Fodran, T., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garcia, B., Vegas, A. L. G., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., Berisso, M. G., Vitale, P. F. G., Gongora, J. P., Gonzalez, J. M., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Khakurdikar, A., Covilakam, V. V. K., Klages, H. O., Kleifges, M., Kleinfeller, J., Knapp, F., Kunka, N., Lago, B. L., Langner, N., De Oliveira, M. A. L., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Presti, D. L., Lopes, L., Lopez, R., Lu, L., Luce, Q., Lundquist, J. P., Payeras, A. M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariani, F. M., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinelli, S., Martinez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mayotte, S., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morejon, L., Morello, C., Mostafa, M., Muller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Nicora, G., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Norwood, I., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nunez, L. A., Oliveira, C., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pawlowsky, J., Pech, M., P Copyrightkala, J., Pelayo, R., Pena-Rodriguez, J., Martins, E. E. P., Armand, J. P., Bertolli, C. P., Perrone, L., Petrera, S., Petrucci, C., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., De Carvalho, W. R., Rojo, J. R., Roncoroni, M. J., Rossoni, S., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saftoiu, A., Saharan, M., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. S., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schafer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schoorlemmer, H., Schovanek, P., Schroder, F. G., Schulte, J., Schulz, T., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smau, R., Smida, R., Sommers, P., Soriano, J. F., Squartini, R., Stadelmaier, M., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Streich, A., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Szadkowski, Z., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Peixoto, C. J. T., Tome, B., Torres, Z., Travaini, A., Travnicek, P., Trimarelli, C., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Galicia, J. F. V., Valore, L., Varela, E., Vasquez-Ramirez, A., Veberic, D., Ventura, C., Quispe, I. D. V., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weindl, A., Wiencke, L., Wilczynski, H., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., and Zehrer, L.
Subjects: Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, UHE, Particle astrophysics, Ultra-high-energy cosmic radiation, Cosmic ray showers, Non-thermal radiation sources, Multivariate analysis, Computer Science::Systems and Control, Cosmic-ray showers (327), High Energy Physics, Particle astrophysics (96), photon: flux, Engineering & allied operations, astro-ph.HE, flux [photon], High Energy Astrophysical Phenomena (astro-ph.HE), energy: high, hybrid, OBSERVATÓRIOS, Astrophysics::Instrumentation and Methods for Astrophysics, Non-thermal radiation sources (1119), Ultra-high-energy cosmic radiation (1733), Astronomy and Astrophysics, Auger, observatory, cosmic radiation, gamma ray, Space and Planetary Science, Experimental High Energy Physics, Multivariate analysis (1913), ddc:520, high [energy], ddc:620, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Ultra-high-energy photons with energies exceeding 1017 eV offer a wealth of connections to different aspects of cosmic-ray astrophysics as well as to gamma-ray and neutrino astronomy. The recent observations of photons with energies in the 1015 eV range further motivate searches for even higher-energy photons. In this paper, we present a search for photons with energies exceeding 2 × 1017 eV using about 5.5 yr of hybrid data from the low-energy extensions of the Pierre Auger Observatory. The upper limits on the integral photon flux derived here are the most stringent ones to date in the energy region between 1017 and 1018 eV., Argentina-Comision Nacional de Energia Atomica, ANPCyT, Argentina-Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET) Argentina-Gobierno de la Provincia de Mendoza Argentina-Municipalidad de Malargue Argentina-NDM Holdings, Australian Research Council, Belgium-Fonds de la Recherche Scientifique (FNRS), FWO, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPQ) Fundacao de Apoio a Pesquisa do Distrito Federal (FAPDF) Brazil-Financiadora de Estudos e Projetos (FINEP) Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio De Janeiro (FAPERJ) Brazil-Sao Paulo Research Foundation (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3 Brazil-Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC), France-Centre de Calcul IN2P3/CNRS Centre National de la Recherche Scientifique (CNRS) France-Conseil Regional Ile-deFrance France-Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS) France-Departement Sciences de l'Univers (SDU-INSU/CNRS) France-Institut Lagrange de Paris (ILP) LABEX ANR-10-LABX-63 ANR-11-IDEX-0004-02, Federal Ministry of Education & Research (BMBF) German Research Foundation (DFG) Germany-Finanzministerium Baden-Wurttemberg Germany-Helmholtz Alliance for Astroparticle Physics (HAP) Germany-Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF) Germany-Ministerium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen Germany-Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg, Italy-Istituto Nazionale di Fisica Nucleare (INFN) Italy-Istituto Nazionale di Astrofisica (INAF) Italy-Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR) Italy-CETEMPS Center of Excellence Italy-Ministero degli Affari Esteri (MAE), Consejo Nacional de Ciencia y Tecnologia (CONACyT) 167733, Mexico-Universidad Nacional Autonoma de Mexico (UNAM) Mexico-PAPIIT DGAPA-UNAM, The Netherlands-Ministry of Education, Culture and Science The Netherlands-Netherlands Organisation for Scientific Research (NWO) The Netherlands-Dutch national e-infrastructure The Netherlands-SURF Cooperative, Poland -Ministry of Education and Science DIR/WK/2018/11 Poland -National Science Centre 2016/22/M/ST9/00198 2016/23/B/ST9/01635 2020/39/B/ST9/01398, Portuguese Foundation for Science and Technology Portugal-FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE), Romania-Ministry of Research, Innovation and Digitization, CNCS/CCCDI-UEFISCDI, within PNCDI III PN19150201/16N/2019 PN1906010 TE128 PED289, Slovenian Research Agency - Slovenia P1-0031 P1-0385 I0-0033 N1-0111, Spanish Government FPA2017-85114-P PID-2019104676GB-C32, Spain-Xunta de Galicia ED431C 2017/07 Spain-Junta de Andalucia Feder Funds SOMM17/6104/UGR P18-FR-4314 Spain-RENATA Red Nacional Tematica de Astroparticulas FPA2015-68783-REDT Spain-Maria de Maeztu Unit of Excellence MDM-2016-0692, United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DE-FG02-99ER41107 DE-SC0011689, National Science Foundation (NSF) 0450696, USA-Grainger Foundation USA-Marie Curie-IRSES/EPLANET USA-European Particle Physics Latin American Network USA-UNESCO, Argentina-Valle Las Lenas MSMT CR LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422
Published: 2022
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7. The relationship of lightning radio pulse amplitudes and source altitudes as observed by LOFAR

Author: A. Nelles, Arthur Corstanje, Heino Falcke, Brian Hare, Stijn Buitink, Katie Mulrey, H. Pandya, J. G. O. Machado, T. Huege, Olaf Scholten, Satyendra Thoudam, G. K. Krampah, Pragati Mitra, S. ter Veen, Tobias Winchen, T. N. G. Trinh, Jörg P. Rachen, Jörg R. Hörandel, Astronomy, Astronomy and Astrophysics Research Group, Physics, and Faculty of Sciences and Bioengineering Sciences
Subjects: Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Cosmology and Extragalactic Astrophysics, Environmental Science (miscellaneous), radio astronomy, Atmosphere, Flash (photography), Altitude, ddc:550, ddc:530, Physics::Atmospheric and Oceanic Physics, amplitude, Physics, pulse detection, Astrophysics::Instrumentation and Methods for Astrophysics, LOFAR, Lightning, Pulse (physics), Amplitude, Physics::Space Physics, General Earth and Planetary Sciences, lightning, Radio astronomy, altitude
Abstract: Earth and Space Science 9(4), e2021EA001958 (2022). doi:10.1029/2021EA001958, When a lightning flash is propagating in the atmosphere it is known that especially the negative leaders emit a large number of very high frequency (VHF) radio pulses. It is thought that this is due to streamer activity at the tip of the growing negative leader. In this work, we have investigated the dependence of the strength of this VHF emission on the altitude of such emission for two lightning flashes as observed by the Low Frequency ARray (LOFAR) radio telescope. We find for these two flashes that the extracted amplitude distributions are consistent with a power-law, and that the amplitude of the radio emissions decreases very strongly with source altitude, by more than a factor of 2 from 1 km altitude up to 5 km altitude. In addition, we do not find any dependence on the extracted power-law with altitude, and that the extracted power-law slope has an average around 3, for both flashes., Published by American Geophysical Union, Malden, Mass.
Published: 2021
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8. Deep-learning based reconstruction of the shower maximum X max using the water-Cherenkov detectors of the Pierre Auger Observatory

Author: A. Segreto, Günter Sigl, Orazio Zapparrata, P. Stassi, Radomir Smida, A. Machado Payeras, G. Cataldi, V. Scherini, Carola Dobrigkeit, M. Muzio, Marcio Aparecido Muller, Srijan Sehgal, Fernando Gollan, Carla Bleve, Rodrigo Guedes Lang, M. E. Bertaina, F. de Palma, Alan Watson, M. Perlin, Mihai Niculescu-Oglinzanu, L. Valore, Belén Andrada, Marina Scornavacche, V. de Souza, G. Golup, Violet M. Harvey, D. Harari, N. Kunka, T. Bister, F. Riehn, P. Tobiska, Jonathan Biteau, M. I. Micheletti, A. Insolia, Jesús Peña-Rodríguez, Matías J. Roncoroni, Sullivan Marafico, M. Kleifges, D. Zavrtanik, Marco Giammarchi, R.J. Barreira Luz, D. Melo, G. P. Guedes, F. Salamida, N. Fazzini, Jonas Glombitza, F. C. T. Barbato, A. Yushkov, Alina Mihaela Badescu, Ioana Codrina Maris, R. Sato, Lourenco Lopes, Toshihiro Fujii, S. Schröder, Italo Epicoco, Marvin Gottowik, Cristina Galea, M. Prouza, Brian Fick, Xavier Bertou, A. Di Matteo, Julian Kemp, Eric Mayotte, D. Nitz, Esteban Roulet, P. Abreu, D. Ravignani, R. M. de Almeida, K. H. Kampert, J. C. Arteaga Velázquez, J. Kleinfeller, A. Zepeda, M. Gómez Berisso, R. C. Shellard, Roberto Mussa, A. Puyleart, Jakub Juryšek, Petr Hamal, Steffen Hahn, Juan Carlos D'Olivo, Julien Manshanden, Lorenzo Caccianiga, Pedro Assis, H. Martinez, A. Etchegoyen, G. C. Hill, Corinne Berat, M. Giller, Jan Pękala, Rúben Conceição, Valerio Verzi, B. Tome, J. Chudoba, L. Lu, H. J. Mathes, Stanislav Michal, B. Wundheiler, Andres Travaini, K. Choi, Alex Kääpä, Ralph Engel, Flavia Gesualdi, J. Perez Armand, E. Varela, D. Correia dos Santos, J. Ridky, L. R. Wiencke, T. Pierog, François Montanet, Justin M. Albury, P. L. Ghia, Marcel Köpke, M. Platino, J.D. Sanabria Gomez, Rodrigo Pelayo, Jose J. Gonzalez, Stijn Buitink, Katie Mulrey, Carlos Escobar, G. De Mauro, Kevin-Druis Merenda, Vladimir Lenok, L. Perrone, H. Schieler, C. J. Todero Peixoto, Mario Buscemi, D. Nosek, E. Santos, Niklas Langner, Antonella Castellina, Eleonora Guido, Antonio Condorelli, M. Risse, Jörg R. Hörandel, J. F. Valdés Galicia, I. De Mitri, Jonathan Blazek, Jose Chinellato, J. Rodriguez Rojo, Fridtjof Feldbusch, A.L. Garcia Vegas, Enrique Zas, I. Lhenry-Yvon, C. Trimarelli, Gaia Silli, A. Filipčič, A.D. Supanitsky, Philipp Papenbreer, Claudio Galelli, A. Weindl, M. Suárez-Durán, J. Stasielak, T. Huege, Hernán Gonzalo Asorey, L. Nellen, L. Anchordoqui, Alena Bakalova, C. Morello, Miroslav Hrabovský, Petr Travnicek, Trent D. Grubb, G. Parente, Fabrizia Canfora, Fernando Contreras, A. Haungs, Juan Manuel Figueira, Roberta Colalillo, Paul Sommers, Clara Keiko Oliveira Watanabe, B. García, M. Schimp, A. G. Mariazzi, R. López, Karen S. Caballero-Mora, H. Wilczyński, Ioana Caracas, A. Letessier-Selvon, Lorenzo Cazon, C. Pérez Bertolli, F. Sanchez, F. Sarazin, S. Petrera, Marc Weber, David Schmidt, G. Farrar, L. Zehrer, J. de Oliveira, Alejandro Almela, P. Mantsch, Z. Szadkowski, M. Schimassek, C. Hojvat, Jan Ebr, Jacco Vink, Peter L. Biermann, L. Bonneau Arbeletche, Maximilian Reininghaus, Paolo Privitera, M. A. Leigui de Oliveira, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, Martin Erdmann, J. de Jesús, A. Taboada, G. Marsella, E. M. Santos, A. Gorgi, H.O. Klages, B. C. Manning, Dariusz Gora, Bjarni Pont, Thomas Bretz, Petr Janecek, Corbin Covault, Matías Rolf Hampel, Frank G. Schröder, R. Squartini, Alfred Müller, P.F. Gómez Vitale, A. Streich, Gioacchino Alex Anastasi, M. Wirtz, David Wittkowski, G. Salina, Roger W Clay, Olivier Deligny, W. M. Namasaka, M. Mastrodicasa, A. C. Rovero, Alexandru Balaceanu, A. A. Nucita, Alan Coleman, Lino Miramonti, S. J. Saffi, Lukáš Vaclavek, J. F. Soriano, D. de Oliveira Franco, R. Alves Batista, Bruce R. Dawson, Octavian Sima, Ana Martina Botti, Jeffrey Brack, Olaf Scholten, P.O. Mazur, K.-H. Becker, Maria Rita Coluccia, Dusan Mandat, Francesco Fenu, Humberto Ibarguen Salazar, M. Pimenta, Tomáš Fodran, Alina Nasr-Esfahani, P.R. Araújo Ferreira, Tobias Winchen, G. Mancarella, B. Keilhauer, Florian Lukas Briechle, Darko Veberič, Ugo Giaccari, S. J. Sciutto, F. Pedreira, Christian Sarmiento-Cano, Raul Sarmento, G. Medina-Tanco, Felix Schlüter, P. Ruehl, Carla Aramo, Vincenzo Rizi, C. J.W.P. Timmermans, Julien Souchard, Jon Paul Lundquist, A. Menshikov, D. Martello, Juan Miguel Carceller, C. M. Schäfer, Markus Roth, Silvia Mollerach, O. Martínez Bravo, Isabel Goos, D. Heck, A. Tapia, Josina Schulte, Peter Hansen, M. del Río, H. Gemmeke, Fabian Gobbi, B. L. Lago, P. Savina, W. Rodrigues de Carvalho, Denise Boncioli, M. Unger, F. Guarino, John Matthews, Peter Buchholz, Marco Aglietta, Miguel Mostafa, E.E. Pereira Martins, Serguei Vorobiov, Martina Bohacova, Miroslav Pech, M. Pothast, J. Hulsman, J. Rautenberg, Pavel Horvath, Q. Luce, Marcus Niechciol, Juan Pablo Gongora, Paula Gina Isar, Sofia Andringa, Maximilian Stadelmaier, Nataliia Borodai, Marcos Cerda, D. Lo Presti, S. J. De Jong, Samo Stanič, Jarryd A. Day, A. Saftoiu, A.C. Cobos Cerutti, Martin Vacula, J. R. T. de Mello Neto, V. Novotny, V. K.C. Varma, Rossella Caruso, A. Lucero, Fernando Catalani, N. González, Kai Daumiller, Heino Falcke, S. Querchfeld, Olena Tkachenko, Thomas Hebbeker, Sergio Dasso, Tristan Sudholz, J. Šupík, Carlo Ventura, Martín Miguel Freire, V. Pirronello, J. Vicha, Ladislav Chytka, A. Aab, Carla Taricco, Matias Tueros, Luis A. Nunez, T. Suomijärvi, J. Pallotta, Hernan Wahlberg, A. Parra, A. Fuster, M. Trini, P.G. Brichetto Orchera, I. Allekotte, A. C. Fauth, Carla Bonifazi, Jose A. Bellido, Fabio Convenga, I.D. Vergara Quispe, M. Zavrtanik, E. De Vito, Giovanni Consolati, Petr Schovanek, Denis Stanca, Ralf Ulrich, L. Nožka, G. Matthiae, Antonio Bueno, Gualberto Avila, John Farmer, Maria-Teresa Dova, R.C. dos Anjos, Adriana Vásquez-Ramírez, M. Palatka, Jeffrey A. Johnsen, Aab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., Alvarez-Mu??iz, J., Alves Batista, R., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Ara??jo Ferreira, P. R., Arteaga Vel??zquez, J. C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Bister, T., Biteau, J., Blazek, J., Bleve, C., Boh????ov??, M., Boncioli, D., Bonifazi, C., Bonneau Arbeletche, L., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Brichetto Orchera, P. G., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Concei????o, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Correia dos Santos, D., Covault, C. E., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jes??s, J., de Jong, S. J., De Mauro, G., de Mello Neto, J. R. T., De Mitri, I., de Oliveira, J., de Oliveira Franco, D., de Palma, F., de Souza, V., De Vito, E., del R??o, M., Deligny, O., Di Matteo, A., Dobrigkeit, C., D'Olivo, J. C., dos Anjos, R. C., Dova, M. T., Ebr, J., Engel, R., Epicoco, I., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filip??i??, A., Fodran, T., Freire, M. M., Fujii, T., Fuster, A., Galea, C., Galelli, C., Garc??a, B., Garcia Vegas, A. L., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glombitza, J., Gobbi, F., Gollan, F., Golup, G., G??mez Berisso, M., G??mez Vitale, P. F., Gongora, J. P., Gonz??lez, J. M., Gonz??lez, N., Goos, I., G??ra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Hamal, P., Hampel, M. R., Hansen, P., Harari, D., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Hill, G. C., Hojvat, C., H??randel, J. R., Horvath, P., Hrabovsk??, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Janecek, P., Johnsen, J. A., Jurysek, J., K????p??, A., Kampert, K. H., Keilhauer, B., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., K??pke, M., Kunka, N., Lago, B. L., Lang, R. G., Langner, N., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., L??pez, R., Lu, L., Luce, Q., Lucero, A., Lundquist, J. P., Machado Payeras, A., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Marafico, S., Mariazzi, A. G., Mari??, I. C., Marsella, G., Martello, D., Martinez, H., Mart??nez Bravo, O., Mastrodicasa, M., Mathes, H. J., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mollerach, S., Montanet, F., Morello, C., Mostaf??, M., M??ller, A. L., Muller, M. A., Mulrey, K., Mussa, R., Muzio, M., Namasaka, W. M., Nasr-Esfahani, A., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., No??ka, L., Nucita, A., N????ez, L. A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., P??kala, J., Pelayo, R., Pe??a-Rodriguez, J., Pereira Martins, E. E., Perez Armand, J., P??rez Bertolli, C., Perlin, M., Perrone, L., Petrera, S., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Pont, B., Pothast, M., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., S??nchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Sch??fer, C. M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schl??ter, F., Schmidt, D., Scholten, O., Schov??nek, P., Schr??der, F. G., Schr??der, S., Schulte, J., Sciutto, S. J., Scornavacche, M., Segreto, A., Sehgal, S., Shellard, R. C., Sigl, G., Silli, G., Sima, O., m??da, R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stani??, S., Stasielak, J., Stassi, P., Streich, A., Su??rez-Dur??n, M., Sudholz, T., Suomij??rvi, T., Supanitsky, A. D., up??k, J., Szadkowski, Z., Taboada, A., Tapia, A., Taricco, C., Timmermans, C., Tkachenko, O., Tobiska, P., Todero Peixoto, C. J., Tom??, B., Travaini, A., Travnicek, P., Trimarelli, C., Trini, M., Tueros, M., Ulrich, R., Unger, M., Vaclavek, L., Vacula, M., Galicia, J. F. Vald??s., Valore, L., Varela, E., Varma K. C., V., V??squez-Ram??rez, A., Veberi??, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Vink, J., Vorobiov, S., Wahlberg, H., Watanabe, C., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczy??ski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yushkov, A., Zapparrata, O., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., High Energy Astrophys. & Astropart. Phys (API, FNWI), Gravitation and Astroparticle Physics Amsterdam, Astronomy and Astrophysics Research Group, Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Aab A., Abreu P., Aglietta M., Albury J.M., Allekotte I., Almela A., Alvarez-Muniz J., Batista R.A., Anastasi G.A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Ferreira P.R.A., Velazquez J.C.A., Asorey H., Assis P., Avila G., Badescu A.M., Bakalova A., Balaceanu A., Barbato F., Luz R.J.B., Becker K.H., Bellido J.A., Berat C., Bertaina M.E., Bertou X., Biermann P.L., Bister T., Biteau J., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Arbeletche L.B., Borodai N., Botti A.M., Brack J., Bretz T., Orchera P.G.B., Briechle F.L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K.S., Caccianiga L., Canfora F., Caracas I., Carceller J.M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J.A., Choi K., Chudoba J., Chytka L., Clay R.W., Cerutti A.C.C., Colalillo R., Coleman A., Coluccia M.R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., dos Santos D.C., Covault C.E., Dasso S., Daumiller K., Dawson B.R., Day J.A., de Almeida R.M., de Jesus J., de Jong S.J., de Mauro G., de Mello Neto J.R.T., de Mitri I., de Oliveira J., de Oliveira Franco D., de Palma F., de Souza V., de Vito E., del Rio M., Deligny O., Di Matteo A., Dobrigkeit C., D'Olivo J.C., dos Anjos R.C., Dova M.T., Ebr J., Engel R., Epicoco I., Erdmann M., Escobar C.O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A.C., Fazzini N., Feldbusch F., Fenu F., Fick B., Figueira J.M., Filipcic A., Fodran T., Freire M.M., Fujii T., Fuster A., Galea C., Galelli C., Garcia B., Vegas A.L.G., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P.L., Giaccari U., Giammarchi M., Giller M., Glombitza J., Gobbi F., Gollan F., Golup G., Berisso M.G., Vitale P.F.G., Gongora J.P., Gonzalez J.M., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T.D., Guarino F., Guedes G.P., Guido E., Hahn S., Hamal P., Hampel M.R., Hansen P., Harari D., Harvey V.M., Haungs A., Hebbeker T., Heck D., Hill G.C., Hojvat C., Horandel J.R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P.G., Janecek P., Johnsen J.A., Jurysek J., Kaapa A., Kampert K.H., Keilhauer B., Kemp J., Klages H.O., Kleifges M., Kleinfeller J., Kopke M., Kunka N., Lago B.L., Lang R.G., Langner N., de Oliveira M.A.L., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Presti D.L., Lopes L., Lopez R., Lu L., Luce Q., Lucero A., Lundquist J.P., Payeras A.M., Mancarella G., Mandat D., Manning B.C., Manshanden J., Mantsch P., Marafico S., Mariazzi A.G., Maris I.C., Marsella G., Martello D., Martinez H., Bravo O.M., Mastrodicasa M., Mathes H.J., Matthews J., Matthiae G., Mayotte E., Mazur P.O., Medina-Tanco G., Melo D., Menshikov A., Merenda K.-D., Michal S., Micheletti M.I., Miramonti L., Mollerach S., Montanet F., Morello C., Mostafa M., Muller A.L., Muller M.A., Mulrey K., Mussa R., Muzio M., Namasaka W.M., Nasr-Esfahani A., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L.A., Palatka M., Pallotta J., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pekala J., Pelayo R., Pena-Rodriguez J., Martins E.E.P., Armand J.P., Bertolli C.P., Perlin M., Perrone L., Petrera S., Pierog T., Pimenta M., Pirronello V., Platino M., Pont B., Pothast M., Privitera P., Prouza M., Puyleart A., Querchfeld S., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Rizi V., Rodrigues de Carvalho W., Rojo J.R., Roncoroni M.J., Roth M., Roulet E., Rovero A.C., Ruehl P., Saffi S.J., Saftoiu A., Salamida F., Salazar H., Salina G., Gomez J.D.S., Sanchez F., Santos E.M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schafer C.M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F.G., Schroder S., Schulte J., Sciutto S.J., Scornavacche M., Segreto A., Sehgal S., Shellard R.C., Sigl G., Silli G., Sima O., Smida R., Sommers P., Soriano J.F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A.D., Supik J., Szadkowski Z., Taboada A., Tapia A., Taricco C., Timmermans C., Tkachenko O., Tobiska P., Peixoto C.J.T., Tome B., Travaini A., Travnicek P., Trimarelli C., Trini M., Tueros M., Ulrich R., Unger M., Vaclavek L., Vacula M., Galicia J.F.V., Valore L., Varela E., Varma V.K.C., Vasquez-Ramirez A., Veberic D., Ventura C., Quispe I.D.V., Verzi V., Vicha J., Vink J., Vorobiov S., Wahlberg H., Watanabe C., Watson A.A., Weber M., Weindl A., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yushkov A., Zapparrata O., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Research unit Astroparticle Physics, Alvarez-Muniz, J., Batista, R. A., Ferreira, P. R. A., Velazquez, J. C. A., Luz, R. J. B., Bohacova, M., Arbeletche, L. B., Orchera, P. G. B., Cerutti, A. C. C., Conceicao, R., dos Santos, D. C., de Jesus, J., de Mauro, G., de Mitri, I., de Vito, E., del Rio, M., Filipcic, A., Garcia, B., Vegas, A. L. G., Berisso, M. G., Vitale, P. F. G., Gonzalez, J. M., Gonzalez, N., Gora, D., Horandel, J. R., Hrabovsky, M., Kaapa, A., Kopke, M., de Oliveira, M. A. L., Presti, D. L., Lopez, R., Payeras, A. M., Maris, I. C., Bravo, O. M., Mostafa, M., Muller, A. L., Nozka, L., Nunez, L. A., Pekala, J., Pena-Rodriguez, J., Martins, E. E. P., Armand, J. P., Bertolli, C. P., Rojo, J. R., Gomez, J. D. S., Sanchez, F., Schafer, C. M., Schluter, F., Schovanek, P., Schroder, F. G., Schroder, S., Smida, R., Stanic, S., Suarez-Duran, M., Suomijarvi, T., Supik, J., Peixoto, C. J. T., Tome, B., Galicia, J. F. V., Varma, V. K. C., Vasquez-Ramirez, A., Veberic, D., Quispe, I. D. V., and Wilczynski, H.
Subjects: showers: energy, longitudinal [showers], interaction: model, Physics::Instrumentation and Detectors, Astronomy, Calibration and fitting methods, Cluster finding, Data analysis, Large detector systems for particle and astroparticle physics, Particle identification methods, Pattern recognition, 01 natural sciences, High Energy Physics - Experiment, Auger, High Energy Physics - Experiment (hep-ex), cluster finding, surface [detector], Observatory, Large detector systems, Instrumentation, Mathematical Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Physics, Pattern recognition, cluster finding, calibration and fitting methods, Settore FIS/01 - Fisica Sperimentale, model [interaction], Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Data analysi, calibration and fitting methods, energy [showers], observatory, Pattern recognition, cluster finding, calibration and fitting method, astroparticle physics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, atmosphere [showers], air, neural network, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, Cosmic ray, detector: fluorescence, 0103 physical sciences, ddc:530, High Energy Physics, ddc:610, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], cosmic radiation: UHE, structure, particle physics, network: performance, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Ciencias Exactas, Cherenkov radiation, fluorescence [detector], Pierre Auger Observatory, mass spectrum [nucleus], showers: atmosphere, detector: surface, hep-ex, 010308 nuclear & particles physics, Física, resolution, calibration, Computational physics, performance [network], Cherenkov counter, Air shower, Large detector systems for particle and astroparticle physic, Experimental High Energy Physics, High Energy Physics::Experiment, nucleus: mass spectrum, showers: longitudinal, RAIOS CÓSMICOS, Energy (signal processing), astro-ph.IM
Abstract: The atmospheric depth of the air shower maximum $X_{\mathrm{max}}$ is an observable commonly used for the determination of the nuclear mass composition of ultra-high energy cosmic rays. Direct measurements of $X_{\mathrm{max}}$ are performed using observations of the longitudinal shower development with fluorescence telescopes. At the same time, several methods have been proposed for an indirect estimation of $X_{\mathrm{max}}$ from the characteristics of the shower particles registered with surface detector arrays. In this paper, we present a deep neural network (DNN) for the estimation of $X_{\mathrm{max}}$. The reconstruction relies on the signals induced by shower particles in the ground based water-Cherenkov detectors of the Pierre Auger Observatory. The network architecture features recurrent long short-term memory layers to process the temporal structure of signals and hexagonal convolutions to exploit the symmetry of the surface detector array. We evaluate the performance of the network using air showers simulated with three different hadronic interaction models. Thereafter, we account for long-term detector effects and calibrate the reconstructed $X_{\mathrm{max}}$ using fluorescence measurements. Finally, we show that the event-by-event resolution in the reconstruction of the shower maximum improves with increasing shower energy and reaches less than $25~\mathrm{g/cm^{2}}$ at energies above $2\times 10^{19}~\mathrm{eV}$., Published version, 29 pages, 12 figures
Published: 2021
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9. PRECISION

Author: Peter Scicluna, Francisca Kemper, Roger Wesson, Ralf Siebenmorgen, J. A. D. L. Blommaert, Sebastian Wolf, Physics, Astrophysics, and Astronomy and Astrophysics Research Group
Subjects: Angular momentum, astro-ph.SR, 010504 meteorology & atmospheric sciences, media_common.quotation_subject, astro-ph.GA, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Asymmetry, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Red supergiant, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, media_common, Physics, Earth and Planetary Astrophysics (astro-ph.EP), Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Torus, Astrophysics - Astrophysics of Galaxies, Exoplanet, Azimuth, Stars, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), astro-ph.EP, Astrophysics::Earth and Planetary Astrophysics, Supergiant, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, astro-ph.IM
Abstract: The search for extrasolar planets has driven rapid advances in instrumentation, resulting in cameras such as SPHERE at the VLT, GPI at Gemini South and SCExAO at Subaru, capable of achieving very high contrast ($\sim10^{6}$) around bright stars with small inner working angles ($\sim 0\farcs{1}$). The optimal exploitation of data from these instruments depends on the availability of easy-to-use software to process and analyse their data products. We present a pure-python pipeline, {\sc precision}, which provides fast, memory-efficient reduction of data from the SPHERE/IRDIS near-infrared imager, and can be readily extended to other instruments. We apply {\sc precision} to observations of the extreme red supergiant VX~Sgr, the inner outflow of which is revealed to host complex, asymmetric structure in the near-IR. In addition, optical polarimetric imaging reveals clear extended polarised emission on $\sim0.5^{\prime\prime}$ scales which varies significantly with azimuth, confirming the asymmetry. While not conclusive, this could suggest that the ejecta are confined to a disc or torus, which we are viewing nearly face on, although other non-spherical or clumpy configurations remain possible. VX~Sgr has no known companions, making such a geometry difficult to explain, as there is no obvious source of angular momentum in the system., 13 pages, 5 figures. Accepted by MNRAS
Published: 2020

10. Properties of the Lunar Detection Mode for ZeV-Scale Particles with LOFAR

Author: Anna Nelles, Arthur Corstanje, Olaf Scholten, Heino Falcke, Tobias Winchen, A. Hörandel, Pragati Mitra, T. N. G. Trinh, Brian Hare, Antonio Bonardi, Satyendra Thoudam, Jörg P. Rachen, S. ter Veen, Laura Rossetto, Stijn Buitink, Katie Mulrey, Pim Schellart, Astronomy and Astrophysics Research Group, Physics, and Faculty of Sciences and Bioengineering Sciences
Subjects: Physics, 010308 nuclear & particles physics, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Detector, Mode (statistics), Astrophysics::Instrumentation and Methods for Astrophysics, Flux, Cosmic ray, LOFAR, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Physics::Geophysics, Radio telescope, Particle shower, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, 010303 astronomy & astrophysics, Energy (signal processing)
Abstract: The steep decrease of the flux of ultra-high energy cosmic rays (UHECR) provides a challenge to answer the long standing question about their origin and nature. A significant increase in detector volume may be achieved byemploying Earth’s moon as a detector that is read out using existing Earth-bound radio telescopes by searching for the radio pulses emitted by the particle shower in the lunar rock. In this contribution we will report on the properties of a corresponding detection mode currently under development for the LOFAR Radio telescope.
Published: 2019
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11. Cosmic Ray Mass Measurements with LOFAR

Author: Anna Nelles, Antonio Bonardi, Laura Rossetto, Olaf Scholten, Satyendra Thoudam, Pragati Mitra, Tobias Winchen, Sander ter Veen, Jörg P. Rachen, Jörg R. Hörandel, Heino Falcke, Stijn Buitink, Katie Mulrey, Arthur Corstanje, Pim Schellart, Gia Trinh, J. Emilio Enriquez, Research unit Astroparticle Physics, Physics, Astronomy and Astrophysics Research Group, and Faculty of Sciences and Bioengineering Sciences
Subjects: Physics, Range (particle radiation), 010308 nuclear & particles physics, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, LOFAR, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Physics and Astronomy(all), 01 natural sciences, law.invention, law, 0103 physical sciences, Dipole antenna, Mass analysis, Particle density, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), 010303 astronomy & astrophysics, Energy (signal processing), Dense core
Abstract: In the dense core of LOFAR individual air showers are detected by hundreds of dipole antennas simultaneously. We reconstruct X max by using a hybrid technique that combines a two-dimensional fit of the radio profile to CoREAS simulations and a one-dimensional fit of the particle density distribution. For high-quality detections, the statistical uncertainty on X max is smaller than 20 g/cm 2 . We present results of cosmic-ray mass analysis in the energy regime of 10 17 - 10 17.5 eV. This range is of particular interest as it may harbor the transition from a Galactic to an extragalactic origin of cosmic rays.
Published: 2017

12. TEC, Trigger and Check, preparing LOFAR for Lunar observations

Author: Jörg P. Rachen, Pim Schellart, Jörg R. Hörandel, Sander ter Veen, Olaf Scholten, Laura Rossetto, Katey Mulrey, Heino Falcke, J. Emilio Enriquez, Antonio Bonardi, Satyendra Thoudam, Gia Trinh, Anna Nelles, Stijn Buitink, Pragati Mitra, Tobias Winchen, Arthur Corstanje, Maaijke Mevius, Physics, Astronomy and Astrophysics Research Group, Faculty of Sciences and Bioengineering Sciences, and Research unit Astroparticle Physics
Subjects: Physics, Total electron content, 010308 nuclear & particles physics, Aperture, QC1-999, TEC, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, LOFAR, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Low frequency, Physics and Astronomy(all), 01 natural sciences, Radio telescope, 0103 physical sciences, Neutrino, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: One of the main ways to use radio to detect Ultra High Energy Neutrinos and Cosmic Rays is the Lunar Askaryan technique, that uses the Moon as a target and searches for nanosecond pulses with large radio telescopes. To use low frequency aperture arrays, such as LOFAR and the SKA, pose new challenges and possibilities in detection techniques of short radio pulses and to measure the Total Electron Content (TEC). As a prepatory work, we have used other measurements that use similar techniques, or that can answer a specific question, with the LOFAR radio telescope. This contribution reports on our work on triggering on short radio signals, post-event imaging of radio signals from buffered data and methods to determine the TEC-value.
Published: 2017
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13. Towards real-time identification of cosmic rays with LOw-Frequency ARray radio antennas

Author: Arthur Corstanje, Jörg P. Rachen, Jörg R. Hörandel, Olaf Scholten, Heino Falcke, Antonio Bonardi, Anna Nelles, Pragati Mitra, Pim Schellart, Satyendra Thoudam, Gia Trinh, Tobias Winchen, J. Emilio Enriquez, Sander ter Veen, Stijn Buitink, Katie Mulrey, Laura Rossetto, Research unit Astroparticle Physics, Physics, Astronomy and Astrophysics Research Group, and Faculty of Sciences and Bioengineering Sciences
Subjects: Astronomy, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Physics and Astronomy(all), Radiation, Low frequency, 01 natural sciences, Atmosphere, Background noise, 0103 physical sciences, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Remote sensing, Physics, 010308 nuclear & particles physics, business.industry, Electrical engineering, Astrophysics::Instrumentation and Methods for Astrophysics, LOFAR, Identification (information), Experimental High Energy Physics, Antenna (radio), business
Abstract: Cosmic rays entering the Earth's atmosphere produce Extensive Air Showers, which emit a radio signal through Geo-magnetic radiation and Askaryan emission. At the present time, one of the biggest challenges for assessing the Radio detection as a valuable technique for Cosmic-ray observation is to identify in real-time the very short (less than 100 ns) radio signals over the background noise. In this work, we present the latest updates on the real-time identification of radio signals from Extensive Air Showers by using the data from LOFAR Low Band Antenna stations, which are sensitive in the 30-80 MHz region.
Published: 2017
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14. Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

Author: The Pierre Auger Collaboration, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-Mu��iz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blanco, A., Blazek, J., Bleve, C., Boh��ov��, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobos, Colalillo, R., Coleman, A., Coluccia, M. R., Concei��o, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., De Mauro, G., Neto, J. R. T. de Mello, De Mitri, I., de Oliveira, J., de Souza, V., Debatin, J., del R��o, M., Deligny, O., Dhital, N., Di Matteo, A., Castro, M. L. D��az, Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. dos, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filip��i��, A., Freire, M. M., Fujii, T., Fuster, A., Garc��a, B., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., G��as, D., Glombitza, J., Gobbi, F., Golup, G., Berisso, M. G��mez, Vitale, P. F. G��mez, Gongora, J. P., Gonz��lez, N., Goos, I., G��ra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., H��randel, J. R., Horvath, P., Hrabovsk��, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., K��p��, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kuempel, D., Mezek, G. Kukec, Awad, A. Kuotb, Lago, B. L., LaHurd, D., Lang, R. G., Legumina, R., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Presti, D. Lo, Lopes, L., L��pez, R., Casado, A. L��pez, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Mariazzi, A. G., Mari��, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Mart��nez, Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostaf��, M., M��ller, A. L., Muller, M. A., M��ller, S., Mussa, R., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., No��ka, L., Nucita, A, N��ez, L. A., Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., P��kala, J., Pelayo, R., Pe��a-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Pothast, M., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigues, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. Sanabria, S��nchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schl��ter, F., Schmidt, D., Scholten, O., Schov��nek, P., Schr��der, F. G., Schr��der, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., ��m��da, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stani��, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Su��rez-Dur��n, M., Sudholz, T., Suomij��rvi, T., Supanitsky, A. D., ��up��k, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Tobiska, P., Peixoto, C. J. Todero, Tom��, B., Elipe, G. Torralba, Travaini, A., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Vald��s, Vali��o, I., Valore, L., van Bodegom, P., Berg, A. M. van den, van Vliet, A., Varela, E., C��rdenas, B. Vargas, V��squez-Ram��rez, A., Veberi��, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villase��or, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiede��ski, M., Wiencke, L., Wilczy��ski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Pierre Auger, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-Muñiz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobo, Colalillo, R., Coleman, A., Coluccia, M. R., Conceição, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., Mauro, G. De, Neto, J. R. T. de Mello, Mitri, I. De, de Oliveira, J., de Souza, V., Debatin, J., Río, M. del, Deligny, O., Dhital, N., Matteo, A. Di, Castro, M. L. Díaz, Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. do, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filipčič, A., Freire, M. M., Fujii, T., Fuster, A., García, B., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glombitza, J., Gobbi, F., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, Gongora, J. P., González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., Kääpä, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kuempel, D., Mezek, G. Kukec, Awad, A. Kuotb, Lago, B. L., Lahurd, D., Lang, R. G., Legumina, R., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Presti, D. Lo, Lopes, L., López, R., Casado, A. López, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Martínez, Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafá, M., Müller, A. L., Muller, M. A., Müller, S., Mussa, R., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Nucita, A, Núñez, L. A., Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pȩkala, J., Pelayo, R., Peña-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Pothast, M., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigue, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. Sanabria, Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schlüter, F., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Šmída, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Tobiska, P., Peixoto, C. J. Todero, Tomé, B., Elipe, G. Torralba, Travaini, A., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdé, Valiño, I., Valore, L., Bodegom, P. van, Berg, A. M. van den, Vliet, A. van, Varela, E., Cárdenas, B. Varga, Vásquez-Ramírez, A., Veberič, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villaseñor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiedeński, M., Wiencke, L., Wilczyński, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zuccarello, F., LaHurd, D., Castillo, J. A., Alvarez-Muniz, J., Luz, R. J. B., Bohacova, M., Cerutti, A. C. C., Conceicao, R., De Almeida, R. M., De Jong, S. J., Mauro, G. D., De Mello Neto, J. R. T., Mitri, I. D., De Oliveira, J., De Souza, V., Rio, M. D., Matteo, A. D., Castro, M. L. D., Anjos, R. C. D., Filipcic, A., Garcia, B., Glas, D., Berisso, M. G., Vitale, P. F. G., Gonzalez, N., Gora, D., Horandel, J. R., Hrabovsky, M., Kaapa, A., Mezek, G. K., Awad, A. K., De Oliveira, M. A. L., Presti, D. L., Lopez, R., Casado, A. L., Maris, I. C., Bravo, O. M., Mostafa, M., Muller, A. L., Muller, S., Nozka, L., Nucita, A., Nunez, L. A., Pkala, J., Pena-Rodriguez, J., De Carvalho, W. R., Rojo, J. R., Gomez, J. D. S., Sanchez, F., Schluter, F., Schovanek, P., Schroder, F. G., Schroder, S., Smida, R., Stanic, S., Suarez-Duran, M., Suomijarvi, T., Supik, J., Peixoto, C. J. T., Tome, B., Elipe, G. T., Galicia, J. F. V., Valino, I., Bodegom, P. V., Van Den Berg, A. M., Vliet, A. V., Cardenas, B. V., Vasquez-Ramirez, A., Veberic, D., Quispe, I. D. V., Villasenor, L., Wiedenski, M., Wilczynski, H., and Research unit Astroparticle Physics
Subjects: cosmological neutrinos, Astronomy, pole, Flux, Astrophysics, 01 natural sciences, neutrino: flux, cosmic ray experiments, neutrino astronomy, ultra high energy cosmic rays, media_common, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), AIR-SHOWERS, astro-ph.HE, cosmological neutrino, Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, COSMIC-RAYS, neutrino: UHE, Auger, observatory, NEUTRINOS, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, air, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, cosmic ray experiment, FOS: Physical sciences, Declination, Celestial pole, 0103 physical sciences, flux: upper limit, High Energy Physics, DETECTOR, Zenith, Astrophysique, Pierre Auger Observatory, flavor, showers: atmosphere, 010308 nuclear & particles physics, detector: surface, Northern Hemisphere, Astronomy and Astrophysics, Astronomie, sensitivity, Sky, Experimental High Energy Physics, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 1017 eV and 1020 eV from point-like sources across the sky, from close to the Southern Celestial Pole up to 60 in declination, with peak sensitivities at declinations around ∼-53 and ∼+55, and an unmatched sensitivity for arrival directions in the Northern hemisphere. A search has been performed for highly-inclined air showers induced by neutrinos of all flavours with no candidate events found in data taken between 1 Jan 2004 and 31 Aug 2018. Upper limits on the neutrino flux from point-like steady sources have been derived as a function of source declination. An unrivaled sensitivity is achieved in searches for transient sources with emission lasting over an hour or less, if they occur within the field of view corresponding to the zenith angle range between 60 and 95 where the SD of the Pierre Auger Observatory is most sensitive to neutrinos., SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2019
Full Text: View/download PDF

15. The Next-Generation Radio Neutrino Observatory — Multi-Messenger Neutrino Astrophysics at Extreme Energies

Author: Stijn Buitink, Nick van Eijndhoven, Krijn de Vries, Physics, Astronomy and Astrophysics Research Group, and Elementary Particle Physics
Subjects: Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment
Abstract: RNO is the mid-scale discovery instrument designed to make the first observation of neutrinos from the cosmos at extreme energies, with sensitivity well beyond current instrument capabilities. This new observatory will be the largest ground-based neutrino telescope to date, enabling the measurement of neutrinos above 10-1⁶ eV.
Published: 2019

16. Updated Calibration of the LOFAR Low-Band Antennas

Author: Heino Falcke, T.N.G. Trinh, Arthur Corstanje, Tobias Winchen, Pim Schellart, Brian Hare, Satyendra Thoudam, J. P. Rachen, Stijn Buitink, Katie Mulrey, S. ter Veen, Jörg R. Hörandel, Laura Rossetto, Anna Nelles, Olaf Scholten, Pragati Mitra, Antonio Bonardi, Astronomy and Astrophysics Research Group, Physics, and Faculty of Sciences and Bioengineering Sciences
Subjects: Physics, 010308 nuclear & particles physics, QC1-999, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, LOFAR, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Signal chain, Frequency spectrum, law.invention, Telescope, Air shower, law, 0103 physical sciences, Range (statistics), Calibration, 010306 general physics, Energy (signal processing), Remote sensing
Abstract: The LOw-Frequency ARray (LOFAR) telescope measures radio emission from air showers. In order to interpret the data, an absolute, frequency dependent calibration is required. Due to a growing need for a better understanding of the measured frequency spectrum, we revisit the calibration of the LOFAR antennas in the range of 30—80 MHz. Using the galactic radio emission and a detailed model of the LOFAR signal chain, we find a calibration that provides an absolute energy scale and allows us to study frequency dependent features in measured air shower signals.
Published: 2019

17. NuRadioMC - Simulation Code for the Next Generation of Radio Neutrino Detectors

Author: Buitink, Stijn, De Vries, Krijn, Van Eijndhoven, Nicolaas, Winchen, Tobias, Physics, Astronomy and Astrophysics Research Group, and Elementary Particle Physics
Subjects: Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment
Abstract: The detection of astrophysical neutrinos by IceCube has opened a new window for the observation of our universe. The use of antennas for detecting astroparticles has been proven useful and accurate after many years of radio cosmic-ray detections, and will be a valuable asset for increasing the statistics for the detection of neutrinos < 10PeV and reaching out to the highest energies. The radio technique requires realistic and precise simulations of the electric field created after the neutrino interacts with the detector volume, how it propagates through media, and what measurable signal it produces in the detector. With the goal of providing accurate, fast simulations of neutrino-induced electric fields, we have created the NuRadioMC code. It builds on the experience of software used for current radio neutrino and cosmic ray experiments.
Published: 2019

18. Towards an improved mass composition analysis with LOFAR

Author: Corstanje, Arthur, Mulrey, Katharine, Buitink, Stijn, Winchen, Tobias, Hörandel, Jörg, Huege, Tim, Krampah, Godwin Komla, Mitra, Pragati, Pandya, Hershal, Rachen, Jörg Paul, Physics, Astronomy and Astrophysics Research Group, and Faculty of Sciences and Bioengineering Sciences
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics
Abstract: The LOFAR radio telescope measures air showers in the energy range 1017 to 1018 eV. For each measured shower, the depth of shower maximum Xmax is reconstructed by simulating the radio signal for an ensemble of showers using Corsika and CoREAS. Fitting their radio ‘footprints’ on the ground to the measured radio data yields an Xmax estimate to a precision of about 20 g/cm2 . Compared to previous works, we have improved the method in several ways. Local atmospheric data and refractive index profiles are now included into the simulations. The energy estimate and the fitting procedure are now done using the radio signals only, thus limiting systematic uncertainties due to the particle detector array (LORA). Using selection criteria from a more elaborate characterisation of the radio and particle detection, we reduce a composition bias in the Xmax reconstruction. A possible residual bias has been bounded from above. Thus, the systematic uncertainties on hXmaxi have been lowered, reducing an important limiting factor for composition studies at any level of statistics.
Published: 2019

19. The energy scale of cosmic rays detected with LOFAR

Author: Mulrey, Katharine, Buitink, Stijn, Winchen, Tobias, Corstanje, Arthur, Hörandel, Jörg, Huege, Tim, Krampah, Godwin Komla, Mitra, Pragati, Pandya, Hershal, Rachen, Jörg Paul, Physics, Astronomy and Astrophysics Research Group, and Faculty of Sciences and Bioengineering Sciences
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics
Abstract: The LOw-Frequency ARray (LOFAR) measures radio emission from extensive air showers. Precise knowledge of the electric field at each antenna in the 30 − 80 MHz range is obtained using a newly developed, frequency-dependent calibration built on knowledge of the Galactic emission and a detailed model of the signal chain. The energy fluence for each event is then determined, allowing for the calculation of the radiation energy of the air shower. The radiation energy, corrected for geometrical effects, scales quadratically with the energy contained in the electromagnetic component of the air shower. These measurements, combined with predictions that rely only on first-principle electrodynamics, provide an energy estimate for the primary particle. In this contribution we present the radio-based energy scale of cosmic rays detected with LOFAR, and compare it to particle-based energy measurements made using the scintillator array located at the LOFAR core.
Published: 2019

20. Reconstructing air showers with LOFAR using event specific GDAS atmospheres

Author: Mitra, Pragati, Mulrey, Katharine, Buitink, Stijn, Winchen, Tobias, Corstanje, Arthur, Hörandel, Jörg, Huege, Tim, Krampah, Godwin Komla, Pandya, Hershal, Rachen, Jörg Paul, Physics, Astronomy and Astrophysics Research Group, and Faculty of Sciences and Bioengineering Sciences
Abstract: Estimating the depth of shower maximum Xmax with high precision is of great interest for the study of primary particle composition. One of the systematic uncertainties in reconstructing Xmax from the radio emission of air showers is the limited knowledge of the atmospheric parameters like humidity, pressure, temperature and the index-of refraction. Using the Global Data Assimilation System (GDAS), a global atmospheric model, we have implemented time-dependent realistic atmospheric profiles in the air shower simulation codes CORSIKA and the radio plug-in CoREAS. This program is now available within CORSIKA and flexible to be adapted for different air shower experiments. We have analyzed the LOFAR cosmic ray data with dedicated simulations for each detected air shower with event specific GDAS atmospheres and investigated the effects of pressure and humidity on the reconstructed Xmax. This study shows that for bulk of the events, where the ground pressure is close to US standard atmosphere values, there is a small systematic shift in Xmax that is less than 2 g/cm2 and for very low pressure values the shift is up to 15 g/cm2 .
Published: 2019

21. Extension of the LOFAR Radboud Air Shower Array

Author: Mulrey, Katharine, Buitink, Stijn, Winchen, Tobias, Corstanje, Arthur, Hörandel, Jörg, Huege, Tim, Krampah, Godwin Komla, Mitra, Pragati, Pandya, Hershal, Rachen, Jörg Paul, Physics, Astronomy and Astrophysics Research Group, and Faculty of Sciences and Bioengineering Sciences
Subjects: Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment
Abstract: The detection of astrophysical neutrinos by IceCube has opened a new window for the observation of our universe. The use of antennas for detecting astroparticles has been proven useful and accurate after many years of radio cosmic-ray detections, and will be a valuable asset for increasing the statistics for the detection of neutrinos < 10PeV and reaching out to the highest energies. The radio technique requires realistic and precise simulations of the electric field created after the neutrino interacts with the detector volume, how it propagates through media, and what measurable signal it produces in the detector. With the goal of providing accurate, fast simulations of neutrino-induced electric fields, we have created the NuRadioMC code. It builds on the experience of software used for current radio neutrino and cosmic ray experiments.
Published: 2019

22. Multi-Messenger Physics With the Pierre Auger Observatory

Author: A. Aab, P. Abreu, M. Aglietta, I. F. M. Albuquerque, J. M. Albury, I. Allekotte, A. Almela, J. Alvarez Castillo, J. Alvarez-Muñiz, G. A. Anastasi, L. Anchordoqui, B. Andrada, S. Andringa, C. Aramo, H. Asorey, P. Assis, G. Avila, A. M. Badescu, A. Bakalova, A. Balaceanu, F. Barbato, R. J. Barreira Luz, S. Baur, K. H. Becker, J. A. Bellido, C. Berat, M. E. Bertaina, X. Bertou, P. L. Biermannb, J. Biteau, S. G. Blaess, A. Blanco, J. Blazek, C. Bleve, M. Boháˇcová, D. Boncioli, C. Bonifazi, N. Borodai, A. M. Botti, J. Bracke, T. Bretz, A. Bridgeman, F. L. Briechle, P. Buchholz, A. Bueno, S. Buitink, M. Buscemi, K. S. Caballero-Mora, L. Caccianiga, L. Calcagni, A. Cancio, F. Canfora, J. M. Carceller, R. Caruso, A. Castellina, F. Catalani, G. Cataldi, L. Cazon, M. Cerda, J. A. Chinellato, J. Chudoba, L. Chytka, R. W. Clay, A. C. Cobos Cerutti, R. Colalillo, A. Coleman, M. R. Coluccia, R. Conceição, A. Condorelli, G. Consolati, F. Contreras, F. Convenga, M. J. Cooper, S. Coutu, C. E. Covault, B. Daniel, S. Dasso, K. Daumiller, B. R. Dawson, J. A. Day, R. M. de Almeida, S. J. de Jong, G. De Mauro, J. R. T. de Mello Neto, I. De Mitri, J. de Oliveira, F. O. de Oliveira Salles, V. de Souza, J. Debatin, M. del Río, O. Deligny, N. Dhital, M. L. Díaz Castro, F. Diogo, C. Dobrigkeit, J. C. D’Olivo, Q. Dorosti, R. C. dos Anjos, M. T. Dova, A. Dundovic, J. Ebr, R. Engel, M. Erdmann, C. O. Escobarc, A. Etchegoyen, H. Falcke, J. Farmer, G. Farrar, A. C. Fauth, N. Fazzinic, F. Feldbusch, F. Fenu, L. P. Ferreyro, J. M. Figueira, A. Filipˇciˇc, M. M. Freire, T. Fujii, f, A. Fuster, B. García, H. Gemmeke, A. Gherghel-Lascu, P. L. Ghia, U. Giaccari, M. Giammarchi, M. Giller, D. Głas, J. Glombitza, F. Gobbi, G. Golup, M. Gómez Berisso, P. F. Gómez Vitale, J. P. Gongora, N. González, I. Goos, D. Góra, A. Gorgi, M. Gottowik, T. D. Grubb, F. Guarino, G. P. Guedes, E. Guido, R. Halliday, M. R. Hampel, P. Hansen, D. Harari, T. A. Harrison, V. M. Harvey, A. Haungs, T. Hebbeker, D. Heck, P. Heimann, G. C. Hill, C. Hojvatc, E. M. Holt, P. Homola, J. R. Hörandel, P. Horvath, M. Hrabovský, T. Huege, J. Hulsman, A. Insolia, P. G. Isar, I. Jandt, J. A. Johnsen, M. Josebachuili, J. Jurysek, A. Kääpä, K. H. Kampert, B. Keilhauer, N. Kemmerich, J. Kemp, H. O. Klages, M. Kleifges, J. Kleinfeller, R. Krause, D. Kuempel, G. Kukec Mezek, A. Kuotb Awad, B. L. Lago, D. LaHurd, R. G. Lang, R. Legumina, M. A. Leigui de Oliveira, V. Lenok, A. Letessier-Selvon, I. Lhenry-Yvon, O. C. Lippmann, D. Lo Presti, L. Lopes, R. López, A. López Casado, R. Lorek, Q. Luce, A. Lucero, M. Malacari, G. Mancarella, D. Mandat, B. C. Manning, P. Mantschc, A. G. Mariazzi, I. C. Mari¸s, G. Marsella, D. Martello, H. Martinez, O. Martínez Bravo, M. Mastrodicasa, H. J. Mathes, S. Mathys, J. Matthews, G. Matthiae, E. Mayotte, P. O. Mazurc, G. Medina-Tanco, D. Melo, A. Menshikov, K. -D. Merenda, S. Michal, M. I. Micheletti, L. Middendorf, L. Miramonti, B. Mitrica, D. Mockler, S. Mollerach, F. Montanet, C. Morello, G. Morlino, M. Mostafá, A. L. Müller, M. A. Muller, d, S. Müller, R. Mussa, L. Nellen, P. H. Nguyen, M. Niculescu-Oglinzanu, M. Niechciol, D. Nitz, g, D. Nosek, V. Novotny, L. Nožka, A Nucita, L. A. Núñez, F. Oikonomou, i, A. Olinto, M. Palatka, J. Pallotta, M. P. Panetta, P. Papenbreer, G. Parente, A. Parra, M. Pech, F. Pedreira, J. Pe¸kala, R. Pelayo, J. Peña-Rodriguez, L. A. S. Pereira, M. Perlin, L. Perrone, C. Peters, S. Petrera, J. Phuntsok, T. Pierog, M. Pimenta, V. Pirronello, M. Platino, J. Poh, B. Pont, C. Porowski, R. R. Prado, P. Privitera, M. Prouza, A. Puyleart, S. Querchfeld, S. Quinn, R. Ramos-Pollan, J. Rautenberg, D. Ravignani, M. Reininghaus, J. Ridky, F. Riehn, M. Risse, P. Ristori, V. Rizi, W. Rodrigues de Carvalho, J. Rodriguez Rojo, M. J. Roncoroni, M. Roth, E. Roulet, A. C. Rovero, P. Ruehl, S. J. Saffi, A. Saftoiu, F. Salamida, H. Salazar, G. Salina, J. D. Sanabria Gomez, F. Sánchez, E. M. Santos, E. Santos, F. Sarazin, R. Sarmento, C. Sarmiento-Cano, R. Sato, P. Savina, M. Schauer, V. Scherini, H. Schieler, M. Schimassek, M. Schimp, F. Schlüter, D. Schmidt, O. Scholten, P. Schovánek, F. G. Schröder, S. Schröder, J. Schumacher, S. J. Sciutto, M. Scornavacche, R. C. Shellard, G. Sigl, G. Silli, O. Sima, h, R. Šmída, G. R. Snow, P. Sommers, J. F. Soriano, J. Souchard, R. Squartini, D. Stanca, S. Staniˇc, J. Stasielak, P. Stassi, M. Stolpovskiy, A. Streich, F. Suarez, M. Suárez-Durán, T. Sudholz, T. Suomijärvi, A. D. Supanitsky, J. Šupík, Z. Szadkowski, A. Taboada, O. A. Taborda, A. Tapia, C. Timmermans, C. J. Todero Peixoto, B. Tomé, G. Torralba Elipe, A. Travaini, P. Travnicek, M. Trini, M. Tueros, R. Ulrich, M. Unger, M. Urban, J. F. Valdés Galicia, I. Valiño, L. Valore, P. van Bodegom, A. M. van den Berg, A. van Vliet, E. Varela, B. Vargas Cárdenas, D. Veberiˇc, C. Ventura, I. D. Vergara Quispe, V. Verzi, J. Vicha, L. Villaseñor, J. Vink, S. Vorobiov, H. Wahlberg, A. A. Watsona, M. Weber, A. Weindl, M. Wiede´nski, L. Wiencke, H. Wilczy´nski, T. Winchen, M. Wirtz, D. Wittkowski, B. Wundheiler, L. Yang, A. Yushkov, E. Zas, D. Zavrtanik, M. Zavrtanik, L. Zehrer, A. Zepeda, B. Zimmermann, M. Ziolkowski, Z. Zong, F. Zuccarello, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Alvarez Castillo, J., Alvarez-Muñiz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermannb, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Boháˇcová, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Bracke, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceição, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., De Mauro, G., de Mello Neto, J. R. T., De Mitri, I., de Oliveira, J., de Oliveira Salles, F. O., de Souza, V., Debatin, J., del Río, M., Deligny, O., Dhital, N., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., D’Olivo, J. C., Dorosti, Q., dos Anjos, R. C., Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobarc, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzinic, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filipˇciˇc, A., Freire, M. M., Fujii, T., F, Fuster, A., García, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glombitza, J., Gobbi, F., Golup, G., Gómez Berisso, M., Gómez Vitale, P. F., Gongora, J. P., González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvatc, C., Holt, E. M., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kääpä, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Kukec Mezek, G., Kuotb Awad, A., Lago, B. L., Lahurd, D., Lang, R. G., Legumina, R., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Lo Presti, D., Lopes, L., López, R., López Casado, A., Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Mantschc, P., Mariazzi, A. G., Mari¸s, I. C., Marsella, G., Martello, D., Martinez, H., Martínez Bravo, O., Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazurc, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafá, M., Müller, A. L., Muller, M. A., D, Müller, S., Mussa, R., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., G, Nosek, D., Novotny, V., Nožka, L., Nucita, A, Núñez, L. A., Oikonomou, F., I, Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pe¸kala, J., Pelayo, R., Peña-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanabria Gomez, J. D., Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schlüter, F., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., H, Šmída, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., Staniˇc, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suarez, F., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Todero Peixoto, C. J., Tomé, B., Torralba Elipe, G., Travaini, A., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J. F., Valiño, I., Valore, L., van Bodegom, P., van den Berg, A. M., van Vliet, A., Varela, E., Vargas Cárdenas, B., Veberiˇc, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Villaseñor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watsona, A. A., Weber, M., Weindl, A., Wiede´nski, M., Wiencke, L., Wilczy´nski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Pierre Auger, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Kampert, Karl-Heinz, Alejandro Mostafa, Miguel, Zas, Enrique, Guarino, F, Physics, Astronomy and Astrophysics Research Group, and Elementary Particle Physics
Subjects: HIGH-ENERGY NEUTRINOS, high energy neutrino, Astronomy, compact binary mergers, high energy neutrinos, high energy neutrons, high energy photons, multi-messenger astrophysics, UHECR, astro-ph.HE, PHOTONS, 01 natural sciences, 7. Clean energy, energy [n], lcsh:QB1-991, energy [cosmic radiation], HESS, LIGO, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, AIR-SHOWERS, energy: high, ORIGIN, Astrophysics::Instrumentation and Methods for Astrophysics, high energy photon, DETETORES, COSMIC-RAYS, photon: energy, multi-messenger astrophysic, neutrino: UHE, BURST, UHE [neutrino], Auger, observatory, compact [binary], high [energy], ddc:620, Astrophysics - High Energy Astrophysical Phenomena, performance, radiation: electromagnetic, FLUORESCENCE DETECTOR, lcsh:Astronomy, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], cosmic radiation: energy, FOS: Physical sciences, ACCELERATION, n: energy, high energy neutron, 0103 physical sciences, High Energy Physics, cosmic radiation: UHE, Pierre Auger Observatory, 010308 nuclear & particles physics, lcsh:QC801-809, energy [photon], Astronomy and Astrophysics, Généralités, binary: compact, flux, messenger, electromagnetic [radiation], lcsh:Geophysics. Cosmic physics, VIRGO, correlation, Experimental High Energy Physics, galaxy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: An overview of the multi-messenger capabilities of the Pierre Auger Observatory is presented. The techniques and performance of searching for Ultra-High Energy neutrinos, photons and neutrons are described. Some of the most relevant results are reviewed, such as stringent upper bounds that were placed to a flux of diffuse cosmogenic neutrinos and photons, bounds placed on neutrinos emitted from compact binary mergers that were detected by LIGO and Virgo during their first and second observing runs, as well as searches for high energy photons and neutrons from the Galactic center that constrain the properties of the putative Galactic PeVatron, observed by the H.E.S.S. collaboration. The observation of directional correlations between ultra-high energy cosmic rays and either high energy astrophysical neutrinos or specific source populations, weighted by their electromagnetic radiation, are also discussed. They constitute additional multi-messenger approaches aimed at identifying the sources of high energy cosmic rays., SCOPUS: re.j, info:eu-repo/semantics/published
Published: 2019
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23. Cosmic Ray Physics with the LOFAR Radio Telescope

Author: Tobias Winchen, Anna Nelles, Katharine Mulrey, Jörg R. Hörandel, Heino Falcke, T. N. G. Trinh, Stijn Buitink, Brian Hare, Pragati Mitra, Arthur Corstanje, Jörg P. Rachen, Satyendra Thoudam, S. ter Veen, Laura Rossetto, Pim Schellart, A. Bonardi, Olaf Scholten, Physics, Astronomy and Astrophysics Research Group, Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, and Faculty of Economic and Social Sciences and Solvay Business School
Subjects: History, Precision testing, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Measure (physics), FOS: Physical sciences, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Education, Radio telescope, 0103 physical sciences, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, LOFAR, Computer Science Applications, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, astro-ph.IM
Abstract: The LOFAR radio telescope is able to measure the radio emission from cosmic ray induced air showers with hundreds of individual antennas. This allows for precision testing of the emission mechanisms for the radio signal as well as determination of the depth of shower maximum $X_{\max}$, the shower observable most sensitive to the mass of the primary cosmic ray, to better than 20 g/cm$^2$. With a densely instrumented circular area of roughly 320 m$^2$, LOFAR is targeting for cosmic ray astrophysics in the energy range $10^{16}$ - $10^{18}$ eV. In this contribution we give an overview of the status, recent results, and future plans of cosmic ray detection with the LOFAR radio telescope., Comment: Proceedings of the 26th Extended European Cosmic Ray Symposium (ECRS), Barnaul/Belokurikha, 2018
Published: 2019
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24. Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

Author: The Pierre Auger Collaboration, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, ez-Muñiz, J. Alvar, Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., Castellina, A., talani, F. Ca, Cataldi, G., Cazon, L., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobos, Colalillo, R., Coleman, A., Coluccia, M. R., ição, R. Conce, Condorelli, A., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., Almeida, R. M. d e, de Jong, S. J., De Mauro, G., Neto, J. R. T. de Mello, De Mitri, I., de Oliveira, J., Salles, F. O. de Oliveira, de Souza, V., Debatin, J., Deligny, O., Dhital, N., Castro, M. L. Díaz, Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. dos, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., č, A. Filipči, Freire, M. M., Fujii, T., Fuster, A., García, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glombitza, J., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., lt, E. M. Ho, Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., ek, J. Jurys, Kääpä, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Mezek, G. Kukec, Awad, A. K uotb, Lago, B. L., LaHurd, D., Lang, R. G., Legumina, R., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Presti, D. Lo, Lopes, L., López, R., Casado, A. López, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Mantsch, P., zzi, A. G. Maria, Mariş, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Martínez, Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., te, E. Mayot, Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafá, M., Müller, A. L., Muller, M. A., Müller, S., Mussa, R., Nellen, L., Nguyen, P. H., glinzanu, M. Niculescu-O, Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Nucita, A, Núñez, L. A., Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pękala, J., Pelayo, R., Peña-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J ., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., hfeld, S. Querc, Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., alho, W. Rodrigues de Carv, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., na, G. Sali, Gomez, J. D. Sanabria, Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schlüter, F., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Šmída, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., ič, S. Stan, Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suarez, F., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., ki, Z. Szadkows, Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Peixoto, C. J. Todero, Tomé, B., Elipe, G. Torralba, Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdés, Valiño, I., Valore, L., van Bodegom, P., Berg, A. M. van den, van Vliet, A., Varela, E., Cárdenas, B. Vargas, zquez, R. A. Vá, Veberič, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villaseñor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., indl, A. We, Wiedeński, M., Wiencke, L., Wilczyński, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., anik, M. Zavrt, Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Research unit Astroparticle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Pierre Auger, High Energy Astrophys. & Astropart. Phys (API, FNWI), Gravitation and Astroparticle Physics Amsterdam, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. A., Alvarez-Muniz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. B., Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., De Almeida, R. M., De Jong, S. J., Mauro, G. D., Neto, J. R. T. D. M., Mitri, I. D., De Oliveira, J., Salles, F. O. D. O., De Souza, V., Debatin, J., Deligny, O., Dhital, N., Castro, M. L. D., Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. D., Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filipcic, A., Freire, M. M., Fujii, T., Fuster, A., Garcia, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glas, D., Glombitza, J., Golup, G., Berisso, M. G., Vitale, P. F. G., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Mezek, G. K., Awad, A. K., Lago, B. L., Lahurd, D., Lang, R. G., Legumina, R., De Oliveira, M. A. L., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Presti, D. L., Lopes, L., Lopez, R., Casado, A. L., Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Mantsch, P., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. M., Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafa, M., Muller, A. L., Muller, M. A., Muller, S., Mussa, R., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nunez, L. A., Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pckala, J., Pelayo, R., Pena-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., De Carvalho, W. R., Rojo, J. R., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salina, G., Gomez, J. D. S., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suarez, F., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Supik, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Peixoto, C. J. T., Tome, B., Elipe, G. T., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. V., Valino, I., Valore, L., Bodegom, P. V., Berg, A. M. V. D., Vliet, A. V., Varela, E., Cardenas, B. V., Vazquez, R. A., Veberic, D., Ventura, C., Quispe, I. D. V., Verzi, V., Vicha, J., Villasenor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiedenski, M., Wiencke, L., Wilczynski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Aab A., Abreu P., Aglietta M., Albuquerque I. F. M., Albury J. M., Allekotte I., Almela A., Castillo J. A., Alvarez-Muniz J., Anastasi G. A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Asorey H., Assis P., Avila G., Badescu A. M., Bakalova A., Balaceanu A., Barbato F., Luz R. J. B., Baur S., Becker K. H., Bellido J. A., Berat C., Bertaina M. E., Bertou X., Biermann P. L., Biteau J., Blaess S. G., Blanco A., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Borodai N., Botti A. M., Brack J., Bretz T., Bridgeman A., Briechle F. L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K. S., Caccianiga L., Calcagni L., Cancio A., Canfora F., Carceller J. M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Chinellato J. A., Chudoba J., Chytka L., Clay R. W., Cerutti A. C. C., Colalillo R., Coleman A., Coluccia M. R., Conceicao R., Condorelli A., Consolati G., Contreras F., Cooper M. J., Coutu S., Covault C. E., Daniel B., Dasso S., Daumiller K., Dawson B. R., Day J. A., De Almeida R. M., De Jong S. J., Mauro G. D., Neto J. R. T. D. M., Mitri I. D., De Oliveira J., Salles F. O. D. O., De Souza V., Debatin J., Deligny O., Dhital N., Castro M. L. D., Diogo F., Dobrigkeit C., D'Olivo J. C., Dorosti Q., Anjos R. C. D., Dova M. T., Dundovic A., Ebr J., Engel R., Erdmann M., Escobar C. O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A. C., Fazzini N., Feldbusch F., Fenu F., Ferreyro L. P., Figueira J. M., Filipcic A., Freire M. M., Fujii T., Fuster A., Garcia B., Gemmeke H., Gherghel-Lascu A., Ghia P. L., Giaccari U., Giammarchi M., Giller M., Glas D., Glombitza J., Golup G., Berisso M. G., Vitale P. F. G., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T. D., Guarino F., Guedes G. P., Guido E., Halliday R., Hampel M. R., Hansen P., Harari D., Harrison T. A., Harvey V. M., Haungs A., Hebbeker T., Heck D., Heimann P., Hill G. C., Hojvat C., Holt E. M., Homola P., Horandel J. R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P. G., Jandt I., Johnsen J. A., Josebachuili M., Jurysek J., Kaapa A., Kampert K. H., Keilhauer B., Kemmerich N., Kemp J., Klages H. O., Kleifges M., Kleinfeller J., Krause R., Kuempel D., Mezek G. K., Awad A. K., Lago B. L., Lahurd D., Lang R. G., Legumina R., De Oliveira M. A. L., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lippmann O. C., Presti D. L., Lopes L., Lopez R., Casado A. L., Lorek R., Luce Q., Lucero A., Malacari M., Mancarella G., Mandat D., Manning B. C., Mantsch P., Mariazzi A. G., Maris I. C., Marsella G., Martello D., Martinez H., Bravo O. M., Mastrodicasa M., Mathes H. J., Mathys S., Matthews J., Matthiae G., Mayotte E., Mazur P. O., Medina-Tanco G., Melo D., Menshikov A., Merenda K. -D., Michal S., Micheletti M. I., Middendorf L., Miramonti L., Mitrica B., Mockler D., Mollerach S., Montanet F., Morello C., Morlino G., Mostafa M., Muller A. L., Muller M. A., Muller S., Mussa R., Nellen L., Nguyen P. H., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L. A., Olinto A., Palatka M., Pallotta J., Panetta M. P., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pckala J., Pelayo R., Pena-Rodriguez J., Pereira L. A. S., Perlin M., Perrone L., Peters C., Petrera S., Phuntsok J., Pierog T., Pimenta M., Pirronello V., Platino M., Poh J., Pont B., Porowski C., Prado R. R., Privitera P., Prouza M., Puyleart A., Querchfeld S., Quinn S., Ramos-Pollan R., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Ristori P., Rizi V., De Carvalho W. R., Rojo J. R., Roncoroni M. J., Roth M., Roulet E., Rovero A. C., Ruehl P., Saffi S. J., Saftoiu A., Salamida F., Salazar H., Saleh A., Salina G., Gomez J. D. S., Sanchez F., Santos E. M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schauer M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F. G., Schroder S., Schumacher J., Sciutto S. J., Scornavacche M., Shellard R. C., Sigl G., Silli G., Sima O., Smida R., Snow G. R., Sommers P., Soriano J. F., Souchard J., Squartini R., Stanca D., Stanic S., Stasielak J., Stassi P., Stolpovskiy M., Streich A., Suarez F., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A. D., Supik J., Szadkowski Z., Taboada A., Taborda O. A., Tapia A., Timmermans C., Peixoto C. J. T., Tome B., Elipe G. T., Travnicek P., Trini M., Tueros M., Ulrich R., Unger M., Urban M., Galicia J. F. V., Valino I., Valore L., Bodegom P. V., Berg A. M. V. D., Vliet A. V., Varela E., Cardenas B. V., Vazquez R. A., Veberic D., Ventura C., Quispe I. D. V., Verzi V., Vicha J., Villasenor L., Vink J., Vorobiov S., Wahlberg H., Watson A. A., Weber M., Weindl A., Wiedenski M., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yang L., Yushkov A., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Zimmermann B., Ziolkowski M., Zong Z., and Zuccarello F.
Subjects: p: showers, photon: Cherenkov, interaction: model, Astronomy, Hadron, pi, astro-ph.HE, 01 natural sciences, nitrogen, iron, Parametrization (atmospheric modeling), Monte Carlo, media_common, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Range (particle radiation), photomultiplier, Settore FIS/01 - Fisica Sperimentale, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, DETETORES, cosmic rays detectors, ultra high energy cosmic rays, Astronomy and Astrophysics, Auger, observatory, geometrical, Astrophysics - High Energy Astrophysical Phenomena, asymmetry, longitudinal, Cherenkov counter: water, air, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, helium, nucleus: atmosphere, Asymmetry, 0103 physical sciences, High Energy Physics, cosmic radiation: UHE, cosmic rays detector, FLUORESCENCE, Astrophysique, Pierre Auger Observatory, electron positron, showers: atmosphere, 010308 nuclear & particles physics, background, detector: surface, showers: spatial distribution, parametrization, Astronomie, Computational physics, 13. Climate action, gamma ray, Experimental High Energy Physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Energy (signal processing)
Abstract: The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmospheric depth at the Pierre Auger Observatory. The shapes of profiles are well reproduced by the Gaisser-Hillas parametrization within the range studied, for E>10 17.8 eV .A detailed analysis of the systematic uncertainties is performed using ten years of data and a full detector simulation. The average shape is quantified using two variables related to the width and asymmetry of the profile, and the results are compared with predictions of hadronic interaction models for different primary particles., SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2019
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25. Calibration of the LOFAR low-band antennas using the Galaxy and a model of the signal chain

Author: Olaf Scholten, Heino Falcke, Antonio Bonardi, Tobias Winchen, S. ter Veen, Stijn Buitink, Katie Mulrey, Arthur Corstanje, Pim Schellart, Laura Rossetto, T. N. G. Trinh, Anna Nelles, Satyendra Thoudam, Brian Hare, Jörg R. Hörandel, Pragati Mitra, Jörg P. Rachen, T. Huege, Astronomy and Astrophysics Research Group, Physics, and Elementary Particle Physics
Subjects: Astroparticle physics, Physics, Spectral shape analysis, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, LOFAR, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, Signal, Signal chain, Computational physics, 0103 physical sciences, ddc:540, Calibration, Astrophysics - Instrumentation and Methods for Astrophysics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Energy (signal processing), astro-ph.IM
Abstract: The LOw-Frequency ARray (LOFAR) is used to make precise measurements of radio emission from extensive air showers, yielding information about the primary cosmic ray. Interpreting the measured data requires an absolute and frequency-dependent calibration of the LOFAR system response. This is particularly important for spectral analyses, because the shape of the detected signal holds information about the shower development. We revisit the calibration of the LOFAR antennas in the range of 30 - 80 MHz. Using the Galactic emission and a detailed model of the LOFAR signal chain, we find an improved calibration that provides an absolute energy scale and allows for the study of frequency-dependent features in measured signals. With the new calibration, systematic uncertainties of 13% are reached, and comparisons of the spectral shape of calibrated data with simulations show promising agreement., Comment: 23 pages, 10 figures
Published: 2019
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26. Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

Author: The Pierre Auger Collaboration, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-Mu��iz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blanco, A., Blazek, J., Bleve, C., Boh��ov��, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobos, Colalillo, R., Coleman, A., Coluccia, M. R., Concei��o, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., De Mauro, G., Neto, J. R. T. de Mello, De Mitri, I., de Oliveira, J., de Souza, V., Debatin, J., del R��o, M., Deligny, O., Dhital, N., Di Matteo, A., Castro, M. L. D��az, Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. dos, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filip��i��, A., Freire, M. M., Fujii, T., Fuster, A., Garc��a, B., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., G��as, D., Glombitza, J., Gobbi, F., Golup, G., Berisso, M. G��mez, Vitale, P. F. G��mez, Gongora, J. P., Gonz��lez, N., Goos, I., G��ra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., H��randel, J. R., Horvath, P., Hrabovsk��, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., K��p��, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kuempel, D., Mezek, G. Kukec, Awad, A. Kuotb, Lago, B. L., LaHurd, D., Lang, R. G., Legumina, R., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Presti, D. Lo, Lopes, L., L��pez, R., Casado, A. L��pez, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Mariazzi, A. G., Mari��, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Mart��nez, Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostaf��, M., M��ller, A. L., Muller, M. A., M��ller, S., Mussa, R., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., No��ka, L., Nucita, A, N��ez, L. A., Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., P��kala, J., Pelayo, R., Pe��a-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Pothast, M., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigues, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. Sanabria, S��nchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schl��ter, F., Schmidt, D., Scholten, O., Schov��nek, P., Schr��der, F. G., Schr��der, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., ��m��da, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stani��, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Su��rez-Dur��n, M., Sudholz, T., Suomij��rvi, T., Supanitsky, A. D., ��up��k, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Tobiska, P., Peixoto, C. J. Todero, Tom��, B., Elipe, G. Torralba, Travaini, A., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Vald��s, Vali��o, I., Valore, L., van Bodegom, P., Berg, A. M. van den, van Vliet, A., Varela, E., C��rdenas, B. Vargas, V��squez-Ram��rez, A., Veberi��, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villase��or, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiede��ski, M., Wiencke, L., Wilczy��ski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Pierre Auger, Research unit Astroparticle Physics, Aab A., Abreu P., Aglietta M., Albuquerque I. F. M., Albury J. M., Allekotte I., Almela A., Castillo J. A., Alvarez-Muniz J., Anastasi G. A., Anchordoqui L., Andrada B., Andringa S., Aramo C., Asorey H., Assis P., Avila G., Badescu A. M., Bakalova A., Balaceanu A., Barbato F., Luz R. J. B., Baur S., Becker K. H., Bellido J. A., Berat C., Bertaina M. E., Bertou X., Biermann P. L., Biteau J., Blanco A., Blazek J., Bleve C., Bohacova M., Boncioli D., Bonifazi C., Borodai N., Botti A. M., Brack J., Bretz T., Bridgeman A., Briechle F. L., Buchholz P., Bueno A., Buitink S., Buscemi M., Caballero-Mora K. S., Caccianiga L., Calcagni L., Cancio A., Canfora F., Caracas I., Carceller J. M., Caruso R., Castellina A., Catalani F., Cataldi G., Cazon L., Cerda M., Chinellato J. A., Choi K., Chudoba J., Chytka L., Clay R. W., Cerutti A. C. C., Colalillo R., Coleman A., Coluccia M. R., Conceicao R., Condorelli A., Consolati G., Contreras F., Convenga F., Cooper M. J., Coutu S., Covault C. E., Daniel B., Dasso S., Daumiller K., Dawson B. R., Day J. A., De Almeida R. M., De Jong S. J., Mauro G. D., Neto J. R. T. D. M., Mitri I. D., De Oliveira J., De Souza V., Debatin J., Rio M. D., Deligny O., Dhital N., Matteo A. D., Castro M. L. D., Dobrigkeit C., D'Olivo J. C., Dorosti Q., Anjos R. C. D., Dova M. T., Dundovic A., Ebr J., Engel R., Erdmann M., Escobar C. O., Etchegoyen A., Falcke H., Farmer J., Farrar G., Fauth A. C., Fazzini N., Feldbusch F., Fenu F., Ferreyro L. P., Figueira J. M., Filipcic A., Freire M. M., Fujii T., Fuster A., Garcia B., Gemmeke H., Gesualdi F., Gherghel-Lascu A., Ghia P. L., Giaccari U., Giammarchi M., Giller M., Glas D., Glombitza J., Gobbi F., Golup G., Berisso M. G., Vitale P. F. G., Gongora J. P., Gonzalez N., Goos I., Gora D., Gorgi A., Gottowik M., Grubb T. D., Guarino F., Guedes G. P., Guido E., Hahn S., Halliday R., Hampel M. R., Hansen P., Harari D., Harrison T. A., Harvey V. M., Haungs A., Hebbeker T., Heck D., Heimann P., Hill G. C., Hojvat C., Holt E. M., Homola P., Horandel J. R., Horvath P., Hrabovsky M., Huege T., Hulsman J., Insolia A., Isar P. G., Johnsen J. A., Jurysek J., Kaapa A., Kampert K. H., Keilhauer B., Kemmerich N., Kemp J., Klages H. O., Kleifges M., Kleinfeller J., Kuempel D., Mezek G. K., Awad A. K., Lago B. L., Lahurd D., Lang R. G., Legumina R., De Oliveira M. A. L., Lenok V., Letessier-Selvon A., Lhenry-Yvon I., Lippmann O. C., Presti D. L., Lopes L., Lopez R., Casado A. L., Lorek R., Luce Q., Lucero A., Malacari M., Mancarella G., Mandat D., Manning B. C., Manshanden J., Mantsch P., Mariazzi A. G., Maris I. C., Marsella G., Martello D., Martinez H., Bravo O. M., Mastrodicasa M., Mathes H. J., Mathys S., Matthews J., Matthiae G., Mayotte E., Mazur P. O., Medina-Tanco G., Melo D., Menshikov A., Merenda K. -D., Michal S., Micheletti M. I., Miramonti L., Mockler D., Mollerach S., Montanet F., Morello C., Morlino G., Mostafa M., Muller A. L., Muller M. A., Muller S., Mussa R., Namasaka W. M., Nellen L., Niculescu-Oglinzanu M., Niechciol M., Nitz D., Nosek D., Novotny V., Nozka L., Nucita A., Nunez L. A., Olinto A., Palatka M., Pallotta J., Panetta M. P., Papenbreer P., Parente G., Parra A., Pech M., Pedreira F., Pkala J., Pelayo R., Pena-Rodriguez J., Pereira L. A. S., Perlin M., Perrone L., Peters C., Petrera S., Phuntsok J., Pierog T., Pimenta M., Pirronello V., Platino M., Poh J., Pont B., Porowski C., Pothast M., Prado R. R., Privitera P., Prouza M., Puyleart A., Querchfeld S., Quinn S., Ramos-Pollan R., Rautenberg J., Ravignani D., Reininghaus M., Ridky J., Riehn F., Risse M., Ristori P., Rizi V., De Carvalho W. R., Rojo J. R., Roncoroni M. J., Roth M., Roulet E., Rovero A. C., Ruehl P., Saffi S. J., Saftoiu A., Salamida F., Salazar H., Salina G., Gomez J. D. S., Sanchez F., Santos E. M., Santos E., Sarazin F., Sarmento R., Sarmiento-Cano C., Sato R., Savina P., Schauer M., Scherini V., Schieler H., Schimassek M., Schimp M., Schluter F., Schmidt D., Scholten O., Schovanek P., Schroder F. G., Schroder S., Schumacher J., Sciutto S. J., Scornavacche M., Shellard R. C., Sigl G., Silli G., Sima O., Smida R., Snow G. R., Sommers P., Soriano J. F., Souchard J., Squartini R., Stadelmaier M., Stanca D., Stanic S., Stasielak J., Stassi P., Stolpovskiy M., Streich A., Suarez-Duran M., Sudholz T., Suomijarvi T., Supanitsky A. D., Supik J., Szadkowski Z., Taboada A., Taborda O. A., Tapia A., Timmermans C., Tobiska P., Peixoto C. J. T., Tome B., Elipe G. T., Travaini A., Travnicek P., Trini M., Tueros M., Ulrich R., Unger M., Urban M., Galicia J. F. V., Valino I., Valore L., Bodegom P. V., Berg A. M. V. D., Vliet A. V., Varela E., Cardenas B. V., Vasquez-Ramirez A., Veberic D., Ventura C., Quispe I. D. V., Verzi V., Vicha J., Villasenor L., Vink J., Vorobiov S., Wahlberg H., Watson A. A., Weber M., Weindl A., Wiedenski M., Wiencke L., Wilczynski H., Winchen T., Wirtz M., Wittkowski D., Wundheiler B., Yang L., Yushkov A., Zas E., Zavrtanik D., Zavrtanik M., Zehrer L., Zepeda A., Zimmermann B., Ziolkowski M., Zuccarello F., Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. A., Alvarez-Muniz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Bakalova, A., Balaceanu, A., Barbato, F., Luz, R. J. B., Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blanco, A., Blazek, J., Bleve, C., Bohacova, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Caracas, I., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Cerda, M., Chinellato, J. A., Choi, K., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceicao, R., Condorelli, A., Consolati, G., Contreras, F., Convenga, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., De Almeida, R. M., De Jong, S. J., Mauro, G. D., Neto, J. R. T. D. M., Mitri, I. D., De Oliveira, J., De Souza, V., Debatin, J., Rio, M. D., Deligny, O., Dhital, N., Matteo, A. D., Castro, M. L. D., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. D., Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filipcic, A., Freire, M. M., Fujii, T., Fuster, A., Garcia, B., Gemmeke, H., Gesualdi, F., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glas, D., Glombitza, J., Gobbi, F., Golup, G., Berisso, M. G., Vitale, P. F. G., Gongora, J. P., Gonzalez, N., Goos, I., Gora, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Hahn, S., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Johnsen, J. A., Jurysek, J., Kaapa, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Kuempel, D., Mezek, G. K., Awad, A. K., Lago, B. L., Lahurd, D., Lang, R. G., Legumina, R., De Oliveira, M. A. L., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lippmann, O. C., Presti, D. L., Lopes, L., Lopez, R., Casado, A. L., Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mancarella, G., Mandat, D., Manning, B. C., Manshanden, J., Mantsch, P., Mariazzi, A. G., Maris, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. M., Mastrodicasa, M., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Miramonti, L., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafa, M., Muller, A. L., Muller, M. A., Muller, S., Mussa, R., Namasaka, W. M., Nellen, L., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nozka, L., Nucita, A., Nunez, L. A., Olinto, A., Palatka, M., Pallotta, J., Panetta, M. P., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pkala, J., Pelayo, R., Pena-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Pothast, M., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., De Carvalho, W. R., Rojo, J. R., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Gomez, J. D. S., Sanchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schluter, F., Schmidt, D., Scholten, O., Schovanek, P., Schroder, F. G., Schroder, S., Schumacher, J., Sciutto, S. J., Scornavacche, M., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Smida, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stadelmaier, M., Stanca, D., Stanic, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suarez-Duran, M., Sudholz, T., Suomijarvi, T., Supanitsky, A. D., Supik, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Tobiska, P., Peixoto, C. J. T., Tome, B., Elipe, G. T., Travaini, A., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. V., Valino, I., Valore, L., Bodegom, P. V., Berg, A. M. V. D., Vliet, A. V., Varela, E., Cardenas, B. V., Vasquez-Ramirez, A., Veberic, D., Ventura, C., Quispe, I. D. V., Verzi, V., Vicha, J., Villasenor, L., Vink, J., Vorobiov, S., Wahlberg, H., Watson, A. A., Weber, M., Weindl, A., Wiedenski, M., Wiencke, L., Wilczynski, H., Winchen, T., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zuccarello, F., Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, Castillo, J. Alvarez, Alvarez-Muñiz, J., Luz, R. J. Barreira, Boháčová, M., Cerutti, A. C. Cobo, Conceição, R., de Almeida, R. M., de Jong, S. J., Mauro, G. De, Neto, J. R. T. de Mello, Mitri, I. De, de Oliveira, J., de Souza, V., Río, M. del, Matteo, A. Di, Castro, M. L. Díaz, Anjos, R. C. do, Filipčič, A., García, B., Głas, D., Berisso, M. Gómez, Vitale, P. F. Gómez, González, N., Góra, D., Hörandel, J. R., Hrabovský, M., Kääpä, A., Mezek, G. Kukec, Awad, A. Kuotb, de Oliveira, M. A. Leigui, Presti, D. Lo, López, R., Casado, A. López, Mariş, I. C., Bravo, O. Martínez, Mostafá, M., Müller, A. L., Müller, S., Nožka, L., Nucita, A, Núñez, L. A., Pȩkala, J., Peña-Rodriguez, J., de Carvalho, W. Rodrigue, Rojo, J. Rodriguez, Gomez, J. D. Sanabria, Sánchez, F., Schlüter, F., Schovánek, P., Schröder, F. G., Schröder, S., Šmída, R., Stanič, S., Suárez-Durán, M., Suomijärvi, T., Šupík, J., Peixoto, C. J. Todero, Tomé, B., Elipe, G. Torralba, Galicia, J. F. Valdé, Valiño, I., Bodegom, P. van, Berg, A. M. van den, Vliet, A. van, Cárdenas, B. Varga, Vásquez-Ramírez, A., Veberič, D., Quispe, I. D. Vergara, Villaseñor, L., Wiedeński, M., and Wilczyński, H.
Subjects: cosmological neutrinos, Astronomy, Flux, Astrophysics, 01 natural sciences, 7. Clean energy, cosmic ray experiments, neutrino astronomy, ultra high energy cosmic rays, surface [detector], Ultra-high-energy cosmic ray, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), cosmological neutrino, Settore FIS/01 - Fisica Sperimentale, DETETORES, neutrino: UHE, UHE [neutrino], Auger, observatory, trajectory, neutrino: flavor, Production (computer science), Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, cosmic ray experiment, Cosmic ray, neutrino: production, production [neutrino], TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY, 0103 physical sciences, ddc:530, model [neutrino], High Energy Physics, cosmic radiation: UHE, Zenith, Astrophysique, neutrino: model, Pierre Auger Observatory, SPECTRUM, 010308 nuclear & particles physics, detector: surface, High Energy Physics::Phenomenology, flavor [neutrino], Astronomy and Astrophysics, Astronomie, flux, Experimental High Energy Physics, atmosphere, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Energy (signal processing)
Abstract: Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming τ neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in ∼ 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an Eν -2 spectrum in the energy range 1.0 × 1017 eV -2.5 × 1019 eV is E2 dNν/dEν < 4.4 × 10-9 GeV cm-2 s-1 sr-1, placing strong constraints on several models of neutrino production at EeV energies and on the properties of the sources of ultra-high-energy cosmic rays., SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2019
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27. Needle-like structures discovered on positively charged lightning branches

Author: S. ter Veen, A. W. Gunst, M. A. Garrett, Laura Rossetto, A. J. van der Horst, J.-M. Grießmeier, R. Blaauw, Mark J. Bentum, R. J. van Weeren, Jörg P. Rachen, B. Ciardi, Pietro Zucca, Heino Falcke, R. Pekal, Aleksandar Shulevski, Anna Nelles, P. Maat, M. J. Norden, H. Paas, James M. Anderson, Stijn Buitink, Katie Mulrey, Richard Fallows, M. C. Toribio, J. Sluman, Luitje Koopmans, Olaf Scholten, Oleg Smirnov, Jörg R. Hörandel, Jochen Eislöffel, Roberto Pizzo, Hanna Rothkaehl, H. J. A. Röttgering, Harvey Butcher, P. Zarka, Olaf Wucknitz, Antonia Rowlinson, T. N. G. Trinh, Andrzej Krankowski, S. Duscha, Arthur Corstanje, Tim Huege, I. M. Avruch, Vishambhar Pandey, Ralph A. M. J. Wijers, M. Iacobelli, Pragati Mitra, Jason W. T. Hessels, Matthias Hoeft, A. van Ardenne, Tobias Winchen, Antonio Bonardi, Dominik J. Schwarz, W. N. Brouw, Brian Hare, Michel Tagger, W. Reich, J. W. Broderick, E. de Geus, Pim Schellart, Marcus Brüggen, M. P. van Haarlem, M. Pandey-Pommier, Joseph R. Dwyer, Marian Soida, High Energy Astrophys. & Astropart. Phys (API, FNWI), KVI Center for Advanced Radiation Technology, University of Groningen [Groningen], Radboud university [Nijmegen], Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Netherlands Institute for Radio Astronomy (ASTRON), Astrophysical Institute, Vrije Universiteit Brussel, Vrije Universiteit [Brussels] (VUB), Karlsruher Institut für Technologie (KIT), Milieux aquatiques, écologie et pollutions (UR MALY), Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA), SRON Netherlands Institute for Space Research (SRON), University of Southampton, Kapteyn Astronomical Institute [Groningen], Jacobs University [Bremen], Research School of Astronomy and Astrophysics [Canberra] (RSAA), Australian National University (ANU), Max Planck Institute for Astrophysics, Max-Planck-Gesellschaft, Medstar Research Institute, Thüringer Landessternwarte Tautenburg (TLS), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National d’Études Spatiales [Paris] (CNES), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Leiden Observatory [Leiden], Universiteit Leiden [Leiden], Institute of Geodesy, Center for Information Technology CIT, Université de Groningen, Centre de Recherche Astrophysique de Lyon (CRAL), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École normale supérieure - Lyon (ENS Lyon), Department of Applied Chemistry (DAC), Banaras Hindu University [Varanasi] (BHU), Max-Planck-Institut für Radioastronomie (MPIFR), Space Research Centre of Polish Academy of Sciences (CBK), Polska Akademia Nauk (PAN), Argelander-Institut für Astronomie (AlfA), Rheinische Friedrich-Wilhelms-Universität Bonn, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), European Project: 227610,EC:FP7:ERC,ERC-2008-AdG,LOFAR-AUGER(2009), European Project: 640130,H2020,ERC-2014-STG,LOFAR(2015), Center for Wireless Technology Eindhoven, Electromagnetics, EM for Radio Science Lab, Physics, Elementary Particle Physics, Astronomy and Astrophysics Research Group, Department of Bio-engineering Sciences, Faculty of Sciences and Bioengineering Sciences, Radboud University [Nijmegen], Vrije Universiteit Brussel (VUB), Global Aerospace, Adran Ffiseg, Prifysgol Cymru Aberystwyth, Universiteit Leiden, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Department of Physics the George Washington University, Space Radio-Diagnostic Research Center [Olsztyn], University of Warmia and Mazury [Olsztyn], Polska Akademia Nauk = Polish Academy of Sciences (PAN), Interactions Son Musique Mouvement, Sciences et Technologies de la Musique et du Son (STMS), Institut de Recherche et Coordination Acoustique/Musique (IRCAM)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche et Coordination Acoustique/Musique (IRCAM)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Rhodes University, Grahamstown, Astronomical Institute Anton Pannekoek (AI PANNEKOEK), University of Amsterdam [Amsterdam] (UvA), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-IRCAM-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-IRCAM-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Astronomy, and Research unit Astroparticle Physics
Subjects: [PHYS]Physics [physics], Physics, Multidisciplinary, 010504 meteorology & atmospheric sciences, Astronomy, 010502 geochemistry & geophysics, 01 natural sciences, Lightning, [SDU]Sciences of the Universe [physics], Natural phenomenon, ddc:530, Spatiotemporal resolution, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Initiation point, 0105 earth and related environmental sciences
Abstract: Nature / Physical science 568(7752), 360 - 363 (2019). doi:10.1038/s41586-019-1086-6, Lightning is a dangerous yet poorly understood natural phenomenon. Lightning forms a network of plasma channels propagating away from the initiation point with both positively and negatively charged ends—called positive and negative leaders. Negative leaders propagate in discrete steps, emitting copious radio pulses in the 30–300-megahertz frequency band that can be remotely sensed and imaged with high spatial and temporal resolution. Positive leaders propagate more continuously and thus emit very little high-frequency radiation. Radio emission from positive leaders has nevertheless been mapped, and exhibits a pattern that is different from that of negative leaders. Furthermore, it has been inferred that positive leaders can become transiently disconnected from negative leaders, which may lead to current pulses that both reconnect positive leaders to negative leaders and cause multiple cloud-to-ground lightning events. The disconnection process is thought to be due to negative differential resistance, but this does not explain why the disconnections form primarily on positive leaders, or why the current in cloud-to-ground lightning never goes to zero. Indeed, it is still not understood how positive leaders emit radio-frequency radiation or why they behave differently from negative leaders. Here we report three-dimensional radio interferometric observations of lightning over the Netherlands with unprecedented spatiotemporal resolution. We find small plasma structures—which we call ‘needles’—that are the dominant source of radio emission from the positive leaders. These structures appear to drain charge from the leader, and are probably the reason why positive leaders disconnect from negative ones, and why cloud-to-ground lightning connects to the ground multiple times., Published by Macmillan28177, London
Published: 2019
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28. Status of the Lunar Detection Mode for Cosmic Particles of LOFAR

Author: T. N. G. Trinh, Brian Hare, Satyendra Thoudam, Stijn Buitink, Olaf Scholten, Katharine Mulrey, Anna Nelles, Heino Falcke, Pragati Mitra, Tobias Winchen, Arthur Corstanje, A. Bonardi, S. ter Veen, Laura Rossetto, Pim Schellart, Jörg P. Rachen, Jörg R. Hörandel, Physics, Astronomy and Astrophysics Research Group, Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, and Faculty of Economic and Social Sciences and Solvay Business School
Subjects: History, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Low frequency, 01 natural sciences, Education, Askaryan effect, Radio telescope, 0103 physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, astro-ph.HE, COSMIC cancer database, 010308 nuclear & particles physics, Mode (statistics), Astrophysics::Instrumentation and Methods for Astrophysics, LOFAR, Computer Science Applications, Orders of magnitude (time), Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, astro-ph.IM
Abstract: Cosmic particles hitting Earth's moon produce radio emission via the Askaryan effect. If the resulting radio ns-pulse can be detected by radio telescopes, this technique potentially increases the available collective area for ZeV scale particles by several orders of magnitude compared to current experiments. The LOw Frequency ARray (LOFAR) is the largest radio telescope operating in the optimum frequency regime for this technique. In this contribution, we report on the status of the implementation of the lunar detection mode at LOFAR., Comment: Proceedings of the 26th Extended European Cosmic Ray Symposium (ECRS), Barnaul/Belokurikha, 2018
Published: 2019

29. The cosmic-ray air-shower signal in Askaryan radio detectors

Author: A. O Murchadha, Stijn Buitink, Olaf Scholten, Krijn D. de Vries, Nick van Eijndhoven, Thomas Meures, Research unit Astroparticle Physics, Physics, Elementary Particle Physics, and Astronomy and Astrophysics Research Group
Subjects: Coherent transition radiation, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Flux, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Askaryan effect, Atmosphere, 0103 physical sciences, Neutrinos, Radio detection, 010306 general physics, Cosmic rays, Askaryan radiation, Physics::Atmospheric and Oceanic Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, Air shower, Transition radiation, Astrophysics::Earth and Planetary Astrophysics, Neutrino, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We discuss the radio emission from high-energy cosmic-ray induced air showers hitting Earth’s surface before the cascade has died out in the atmosphere. The induced emission gives rise to a radio signal which should be detectable in the currently operating Askaryan radio detectors built to search for the GZK neutrino flux in ice. The in-air emission, the in-ice emission, as well as a new component, the coherent transition radiation when the particle bunch crosses the air–ice boundary, are included in the calculations.
Published: 2016
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30. Influence of atmospheric electric fields on the radio emission from extensive air showers

Author: Heino Falcke, J. E. Enriquez, Pim Schellart, K. D. de Vries, Jörg P. Rachen, Jörg R. Hörandel, Ute Ebert, A. Nelles, Casper Rutjes, T. N. G. Trinh, Arthur Corstanje, A.M. van den Berg, Satyendra Thoudam, S. ter Veen, Laura Rossetto, Stijn Buitink, Christoph Köhn, Olaf Scholten, Elementary Processes in Gas Discharges, Research unit Astroparticle Physics, Physics, Elementary Particle Physics, and Astronomy and Astrophysics Research Group
Subjects: THUNDERSTORMS, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Radiation, 01 natural sciences, Physics::Geophysics, PHYSICS, Electric field, 0103 physical sciences, 010306 general physics, Physics::Atmospheric and Oceanic Physics, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, FLASHES, Astrophysics::Instrumentation and Methods for Astrophysics, LOFAR, Polarization (waves), SIMULATIONS, Computational physics, MODEL, Physics - Atmospheric and Oceanic Physics, 13. Climate action, Atmospheric and Oceanic Physics (physics.ao-ph), Thunderstorm, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, RADIATION, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The atmospheric electric fields in thunderclouds have been shown to significantly modify the intensity and polarization patterns of the radio footprint of cosmic-ray-induced extensive air showers. Simulations indicated a very nonlinear dependence of the signal strength in the frequency window of 30-80 MHz on the magnitude of the atmospheric electric field. In this work we present an explanation of this dependence based on Monte Carlo simulations, supported by arguments based on electron dynamics in air showers and expressed in terms of a simplified model. We show that by extending the frequency window to lower frequencies, additional sensitivity to the atmospheric electric field is obtained.
Published: 2016
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31. Cosmic-ray energy spectrum and composition up to the ankle: the case for a second Galactic component

Author: Abraham Achterberg, A. van Vliet, Satyendra Thoudam, Stijn Buitink, Jörg P. Rachen, Jörg R. Hörandel, Heino Falcke, Physics, and Astronomy and Astrophysics Research Group
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astronomy, FOS: Physical sciences, chemistry.chemical_element, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, outflows, Auger, Diffusion, cosmic rays, Observatory, 0103 physical sciences, Energy spectrum, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Helium, Astrophysics::Galaxy Astrophysics, ISM: supernova remnants, High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, 010308 nuclear & particles physics, Component (thermodynamics), Astronomy and Astrophysics, Supernova, chemistry, Space and Planetary Science, stars: winds, Astrophysics - High Energy Astrophysical Phenomena, galaxies: ISM
Abstract: We have carried out a detailed study to understand the observed energy spectrum and composition of cosmic rays with energies up to ~10^18 eV. Our study shows that a single Galactic component with subsequent energy cut-offs in the individual spectra of different elements, optimised to explain the observed spectra below ~10^14 eV and the knee in the all-particle spectrum, cannot explain the observed all-particle spectrum above ~2x10^16 eV. We discuss two approaches for a second component of Galactic cosmic rays -- re-acceleration at a Galactic wind termination shock, and supernova explosions of Wolf-Rayet stars, and show that the latter scenario can explain almost all observed features in the all-particle spectrum and the composition up to ~10^18 eV, when combined with a canonical extra-galactic spectrum expected from strong radio galaxies or a source population with similar cosmological evolution. In this two-component Galactic model, the knee at ~ 3x10^15 eV and the second knee at ~10^17 eV in the all-particle spectrum are due to the cut-offs in the first and second components, respectively. We also discuss several variations of the extra-galactic component, from a minimal contribution to scenarios with a significant component below the ankle (at ~4x10^18 eV), and find that extra-galactic contributions in excess of regular source evolution are neither indicated nor in conflict with the existing data. Our main result is that the second Galactic component predicts a composition of Galactic cosmic rays at and above the second knee that largely consists of helium or a mixture of helium and CNO nuclei, with a weak or essentially vanishing iron fraction, in contrast to most common assumptions. This prediction is in agreement with new measurements from LOFAR and the Pierre Auger Observatory which indicate a strong light component and a rather low iron fraction between ~10^17 and 10^18 eV., Added Table 4; Published in A&A, 595 (2016) A33 (Highlight paper)
Published: 2016
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32. On the detection of CO and mass-loss of bulge OH/IR stars

Author: Leen Decin, Martin Groenewegen, Joris Blommaert, Kay Justtanont, Astronomy and Astrophysics Research Group, Physics, and Astrophysics
Subjects: CIRCUMSTELLAR ENVELOPES, FOS: Physical sciences, Astrophysics, stars: AGB and post-AGB, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, GALACTIC BULGE, 01 natural sciences, circumstellar matter, Galaxy: bulge, law.invention, INFRARED-SPECTROSCOPY, Telescope, Radio lines: stars, law, Bulge, OH-IR STARS, 0103 physical sciences, Radiative transfer, Asymptotic giant branch, Astrophysics::Solar and Stellar Astrophysics, Spectroscopy, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, stars [radio lines], Physics, Science & Technology, AGB STARS, DUST SHELLS, 010308 nuclear & particles physics, 1ST DETAILED ABUNDANCES, Astronomy and Astrophysics, mass-loss [stars], Astrophysics - Astrophysics of Galaxies, AGB and post-AGB [stars], Galaxy, bulge [galaxy], Stars, Astrophysics - Solar and Stellar Astrophysics, MIRA VARIABLES, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), ASYMPTOTIC GIANT BRANCH, Physical Sciences, Spectral energy distribution, MILKY-WAY, Astrophysics::Earth and Planetary Astrophysics, stars: mass-loss
Abstract: © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. We report on the successful search forCO(2-1) and (3-2) emission associated with OH/IR stars in the Galactic bulge. We observed a sample of eight extremely red asymptotic giant branch stars with the Atacama Pathfinder EXperiment telescope and detected seven. The sources were selected at a sufficiently high galactic latitude to avoid interference by interstellar CO, which hampered previous studies of inner galaxy stars. To study the nature of our sample and the mass-loss, we constructed the spectral energy distribution (SEDs) from photometric data and Spitzer IRS spectroscopy. In a first step, we apply radiative transfer modelling to fit the SEDs and obtain luminosities and dust mass-loss rates (MLRs). Through dynamical modelling, we then retrieve the total MLR and the gas-to-dust ratios. We derived variability periods of our stars. The luminosities range between approximately 4000 and 5500 L ⊙ and periods are shorter than 700 d. The total MLR ranges between 10 -5 and 10 -4 M ⊙ yr -1 . Comparison with evolutionary models shows that the progenitor mass ≈ 1.5 M ⊙ , similar to the bulge Miras of intermediate age (3 Gyr). The gas-to-dust ratios are between 100 and 400 and are similar to what is found for OH/IR stars in the galactic disc. One star, IRAS 17347-2319, has a very short period of approximately 300 d that may be decreasing further. It may belong to a class of Mira variables with a sudden change in period as observed in some Galactic objects. It would be the first example of an OH/IR star in this class and deserves further follow-up observations. ispartof: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY vol:479 issue:3 pages:3545-3562 status: published
Published: 2018

33. Polycyclic aromatic hydrocarbon emission toward the Galactic bulge

Author: M. J. Shannon, Joris Blommaert, Els Peeters, Jan Cami, Astronomy and Astrophysics Research Group, Physics, and Astrophysics
Subjects: Astrochemistry, 010504 meteorology & atmospheric sciences, molecular data, Astrophysics::High Energy Astrophysical Phenomena, Population, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Spitzer Space Telescope, Bulge, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Continuum (set theory), education, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Line (formation), Physics, infrared: ISM, education.field_of_study, Zodiacal light, astrochemistry, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, ISM: molecules, ISM: lines and bands, Astrophysics - Solar and Stellar Astrophysics, 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Cirrus, Astrophysics::Earth and Planetary Astrophysics, techniques: spectroscopic
Abstract: We examine polycyclic aromatic hydrocarbon (PAH), dust and atomic/molecular emission toward the Galactic bulge using Spitzer Space Telescope observations of four fields: C32, C35, OGLE and NGC 6522. These fields are approximately centered on (l, b) = (0.0{\deg}, 1.0{\deg}), (0.0{\deg}, -1.0{\deg}), (0.4{\deg}, -2.1{\deg}) and (1.0{\deg}, -3.8{\deg}), respectively. Far-infrared photometric observations complement the Spitzer/IRS spectroscopic data and are used to construct spectral energy distributions. We find that the dust and PAH emission are exceptionally similar between C32 and C35 overall, in part explained due to their locations---they reside on or near boundaries of a 7 Myr-old Galactic outflow event and are partly shock-heated. Within the C32 and C35 fields, we identify a region of elevated H{\alpha} emission that is coincident with elevated fine-structure and [O IV] line emission and weak PAH feature strengths. We are likely tracing a transition zone of the outflow into the nascent environment. PAH abundances in these fields are slightly depressed relative to typical ISM values. In the OGLE and NGC 6522 fields, we observe weak features on a continuum dominated by zodiacal dust. SED fitting indicates that thermal dust grains in C32 and C35 have comparable temperatures to those of diffuse, high-latitude cirrus clouds. Little variability is detected in the PAH properties between C32 and C35, indicating that a stable population of PAHs dominates the overall spectral appearance. In fact, their PAH features are exceptionally similar to that of the M82 superwind, emphasizing that we are probing a local Galactic wind environment., Comment: Accepted for publication in the Astrophysical Journal
Published: 2018

34. Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory

Author: The Pierre Auger Collaboration, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-Muñiz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arsene, N., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobos, Colalillo, R., Coleman, A., Collica, L., Coluccia, M. R., Conceição, R., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., D'Amico, S., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., De Mauro, G., Neto, J. R. T. de Mello, De Mitri, I., de Oliveira, J., de Souza, V., Debatin, J., Deligny, O., Dhital, N., Castro, M. L. Díaz, Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. dos, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Fick, B., Figueira, J. M., Filipčič, A., Freire, M. M., Fujii, T., Fuster, A., Gaïor, R., García, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glombitza, J., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kääpä, A., Kambeitz, O., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Mezek, G. Kukec, Kunka, N., Awad, A. Kuotb, Lago, B. L., LaHurd, D., Lang, R. G., Legumina, R., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Presti, D. Lo, Lopes, L., López, R., Casado, A. López, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Martínez, Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina, C., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafá, M., Müller, A. L., Muller, M. A., Müller, S., Mussa, R., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Niemietz, L., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Nucita, A, Núñez, L. A., Oikonomou, F., Olinto, A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pękala, J., Pelayo, R., Peña-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Quel, E. J., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigues, Fernandez, G. Rodriguez, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salina, G., Sánchez, F., Sanchez-Lucas, P., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Schulz, A., Schumacher, J., Sciutto, S. J., Segreto, A., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Šmída, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Strafella, F., Streich, A., Suarez, F., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., Swain, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Timmermans, C., Peixoto, C. J. Todero, Tomé, B., Elipe, G. Torralba, Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdés, Valiño, I., Valore, L., van Bodegom, P., Berg, A. M. van den, van Vliet, A., Varela, E., Cárdenas, B. Vargas, Vázquez, R. A., Veberič, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weindl, A., Wiedeński, M., Wiencke, L., Wilczyński, H., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Pierre Auger, Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-Muñiz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arsene, N., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobo, Colalillo, R., Coleman, A., Collica, L., Coluccia, M. R., Conceição, R., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., D'Amico, S., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., Mauro, G. De, Neto, J. R. T. de Mello, Mitri, I. De, de Oliveira, J., de Souza, V., Debatin, J., Deligny, O., Dhital, N., Castro, M. L. Díaz, Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. do, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Fick, B., Figueira, J. M., Filipčič, A., Freire, M. M., Fujii, T., Fuster, A., Gaïor, R., García, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glombitza, J., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kääpä, A., Kambeitz, O., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Mezek, G. Kukec, Kunka, N., Awad, A. Kuotb, Lago, B. L., Lahurd, D., Lang, R. G., Legumina, R., de Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Presti, D. Lo, Lopes, L., López, R., Casado, A. López, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Martinez, H., Bravo, O. Martínez, Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina, C., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafá, M., Müller, A. L., Muller, M. A., Müller, S., Mussa, R., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Niemietz, L., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Nucita, A, Núñez, L. A., Oikonomou, F., Olinto, A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pȩkala, J., Pelayo, R., Peña-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Quel, E. J., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., de Carvalho, W. Rodrigue, Fernandez, G. Rodriguez, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salina, G., Sánchez, F., Sanchez-Lucas, P., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Schulz, A., Schumacher, J., Sciutto, S. J., Segreto, A., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Šmída, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Strafella, F., Streich, A., Suarez, F., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., Swain, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Timmermans, C., Peixoto, C. J. Todero, Tomé, B., Elipe, G. Torralba, Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdé, Valiño, I., Valore, L., Bodegom, P. van, Berg, A. M. van den, Vliet, A. van, Varela, E., Cárdenas, B. Varga, Vázquez, R. A., Veberič, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weindl, A., Wiedeński, M., Wiencke, L., Wilczyński, H., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., De Almeida, R. M., De Jong, S. J., Neto, J. R. T. De Mello, De Oliveira, J., De Souza, V., Anjos, R. C. Do, De Oliveira, M. A. Leigui, Nucita, A., Pkala, J., De Carvalho, W. Rodrigue, Bodegom, P. Van, Berg, A. M. Van Den, Vliet, A. Van, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Research unit Astroparticle Physics, and LaHurd, D.
Subjects: Physics::Instrumentation and Detectors, Astronomy, engineering, 01 natural sciences, ultra high energy cosmic ray, Auger, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), cosmic ray experiments, cosmic rays detectors, ultra high energy cosmic rays, Astronomy and Astrophysics, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Cosmic ray experiments, cosmic rays detectors, ultra high energy cosmic rays, Astronomy and Astrophysics, Absorption (electromagnetic radiation), Physics, radio wave, Settore FIS/01 - Fisica Sperimentale, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, DETETORES, COSMIC-RAYS, observatory, Amplitude, Astrophysics - Instrumentation and Methods for Astrophysics, numerical calculations: Monte Carlo, air, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, cosmic ray experiment, cascade: electromagnetic, Optics, 0103 physical sciences, High Energy Physics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], cosmic rays detector, 010306 general physics, cosmic ray experiments, cosmic rays detectors, ultra high energy cosmic rays, Instrumentation and Methods for Astrophysics (astro-ph.IM), Zenith, Astrophysique, Pierre Auger Observatory, showers: atmosphere, 010308 nuclear & particles physics, business.industry, Scattering, hep-ex, detector: surface, scattering, Astronomie, Air shower, Experimental High Energy Physics, ARRAY, High Energy Physics::Experiment, EMISSION, business, absorption, astro-ph.IM
Abstract: With the Auger Engineering Radio Array (AERA) of the Pierre Auger Observatory, we have observed the radio emission from 561 extensive air showers with zenith angles between 60 and 84. In contrast to air showers with more vertical incidence, these inclined air showers illuminate large ground areas of several km2 with radio signals detectable in the 30 to 80 MHz band. A comparison of the measured radio-signal amplitudes with Monte Carlo simulations of a subset of 50 events for which we reconstruct the energy using the Auger surface detector shows agreement within the uncertainties of the current analysis. As expected for forward-beamed radio emission undergoing no significant absorption or scattering in the atmosphere, the area illuminated by radio signals grows with the zenith angle of the air shower. Inclined air showers with EeV energies are thus measurable with sparse radio-antenna arrays with grid sizes of a km or more. This is particularly attractive as radio detection provides direct access to the energy in the electromagnetic cascade of an air shower, which in case of inclined air showers is not accessible by arrays of particle detectors on the ground., SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2018
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35. Large-scale Cosmic-Ray Anisotropies above 4 EeV Measured by the Pierre Auger Observatory

Author: Aab, A., Abreu, P., AGLIETTA, MARCO, Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Alvarez Castillo, J., Alvarez-Muñiz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Balaceanu, A., Barbato, F., Barreira Luz, R. J., Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., CASTELLINA, ANTONELLA, Catalani, F., Cataldi, G., Cazon, L., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Coluccia, M. R., Conceição, R., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., de Almeida, R. M., de Jong, S. J., De Mauro, G., de Mello Neto, J. R. T., De Mitri, I., de Oliveira, J., de Souza, V., Debatin, J., Deligny, O., Dhital, N., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., dos Anjos, R. C., Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filipčič, A., Freire, M. M., Fujii, T., Fuster, A., García, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glombitza, J., Golup, G., Gómez Berisso, M., Gómez Vitale, P. F., González, N., Goos, I., Góra, D., GORGI, Alessio, Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kääpä, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Kukec Mezek, G., Kuotb Awad, A., Lago, B. L., LaHurd, D., Lang, R. G., Legumina, R., Leigui de Oliveira, M. A., Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., López, R., López Casado, A., Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mancarella, G., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariș, I. C., Marsella, G., Martello, D., Martinez, H., Martínez Bravo, O., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., MORLINO, GIOVANNI, Mostafá, M., Müller, A. L., Muller, M. A., Müller, S., Mussa, R., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Nucita, A., Núñez, L. A., Olinto, A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pȩkala, J., Pelayo, R., Peña-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Rojo, J., Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salina, G., Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Schumacher, J., Sciutto, S. J., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Šmída, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suarez, F., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Todero Peixoto, C. J., Tomé, B., Torralba Elipe, G., Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J. F., Valiño, I., Valore, L., van Bodegom, P., van den Berg, A. M., van Vliet, A., Varela, E., Vargas Cárdenas, B., Vázquez, R. A., Veberič, D., Ventura, C., Vergara Quispe, I. D., Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Watson, A. A., Weber, M., Weindl, A., Wiedeński, M., Wiencke, L., Wilczyński, H., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, Francesca, Pierre Auger Collaboration, Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-Muñiz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Baur, S., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, C., Boháčová, M., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Calcagni, L., Cancio, A., Canfora, F., Carceller, J. M., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Chinellato, J. A., Chudoba, J., Chytka, L., Clay, R. W., Cerutti, A. C. Cobo, Colalillo, R., Coleman, A., Coluccia, M. R., Conceição, R., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., Almeida, R. M. De, Jong, S. J. De, De Mauro, G., Neto, J. R. T. De Mello, De Mitri, I., Deoliveira, J., De Souza, V., Debatin, J., Deligny, O., Dhital, N., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorosti, Q., Anjos, R. C. Do, Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Escobar, C. O., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Ferreyro, L. P., Figueira, J. M., Filipčič, A., Freire, M. M., Fujii, T., Fuster, A., García, B., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glombitza, J., Golup, G., Berisso, M. Gómez, Vitale, P. F. Gómez, González, N., Goos, I., Góra, D., Gorgi, A., Gottowik, M., Grubb, T. D., Guarino, F., Guedes, G. P., Guido, E., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Hill, G. C., Hojvat, C., Holt, E. M., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Käpä, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., Kemp, J., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kuempel, D., Mezek, G. Kukec, Awad, A. Kuotb, Lago, B. L., Lahurd, D., Lang, R. G., Legumina, R., De Oliveira, M. A. Leigui, Lenok, V., Letessier-Selvon, A., Lhenry-Yvon, I., Lo Presti, D., Lopes, L., López, R., Casado, A. López, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mancarella, G., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariş, I. C., Marsella, G., Martello, D., Martinez, H., Martínez Bravo, O., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafá, M., Müller, A. L., Muller, M. A., Müller, S., Mussa, R., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Nitz, D., Nosek, D., Novotny, V., Nožka, L., Nucita, A., Nñez, L. A., Olinto, A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Pech, M., Pedreira, F., Pkala, J., Pelayo, R., Peña-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Pont, B., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Puyleart, A., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Reininghaus, M., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., De Carvalho, W. Rodrigue, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salina, G., Sánchez, F., Santos, E. M., Santos, E., Sarazin, F., Sarmento, R., Sarmiento-Cano, C., Sato, R., Savina, P., Schauer, M., Scherini, V., Schieler, H., Schimassek, M., Schimp, M., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schröder, S., Schumacher, J., Sciutto, S. J., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Šmída, R., Snow, G. R., Sommers, P., Soriano, J. F., Souchard, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Stassi, P., Stolpovskiy, M., Streich, A., Suarez, F., Suárez-Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Šupík, J., Szadkowski, Z., Taboada, A., Taborda, O. A., Tapia, A., Timmermans, C., Peixoto, C. J. Todero, Tomé, B., Elipe, G. Torralba, Travnicek, P., Trini, M., Tueros, M., Ulrich, R., Unger, M., Urban, M., Galicia, J. F. Valdé, Valiño, I., Valore, L., Bodegom, P. Van, Berg, A. M. Van Den, Vliet, A. Van, Varela, E., Cárdenas, B. Varga, Vázquez, R. A., Veberič, D., Ventura, C., Quispe, I. D. Vergara, Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Watson, A. A., Weber, M., Weindl, A., Wiedeński, M., Wiencke, L., Wilczyński, H., Wirtz, M., Wittkowski, D., Wundheiler, B., Yang, L., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zehrer, L., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, Research unit Astroparticle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Pierre Auger, Almeida, R. M. de, Jong, S. J. de, Mauro, G. De, Neto, J. R. T. de Mello, Mitri, I. De, Oliveira, J. de, Souza, V. de, D’Olivo, J. C., Anjos, R. C. do, Kääpä, A., de Oliveira, M. A. Leigui, Presti, D. Lo, Nucita, A, Núñez, L. A., Pȩkala, J., de Carvalho, W. Rodrigue, Savina, Pierpaolo, Bodegom, P. van, Berg, A. M. van den, Vliet, A. van, LaHurd, D., SAVINA, PIERPAOLO, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: Astronomy, magnetic field, Astrophysics, 01 natural sciences, Amplitude, astroparticle physics, cosmic rays, Anisotropy, 010303 astronomy & astrophysics, cosmic ray, astroparticle physics, cosmic rays, Right ascension, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, astro-ph.HE, COSMIC cancer database, ORIGIN, OBSERVATÓRIOS, Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, astroparticle physic, Auger, Astronomy and Astrophysics, Space and Planetary Science, observatory, modulation, Cosmic cancer database, Astrophysics - High Energy Astrophysical Phenomena, large scale anysotropy, splitting, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Context (language use), cosmic radiation: anisotropy, 0103 physical sciences, High Energy Physics, cosmic radiation: UHE, Pierre auger observatory, Pierre Auger Observatory, extragalactic origin, 010308 nuclear & particles physics, Física, Astronomy and Astrophysic, Dipole, Experimental High Energy Physics, Observatory, Astroparticle physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], large scale anysotropy, extragalactic origin, dipole
Abstract: We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and $E\geq 8$ EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index $\beta=0.79\pm 0.19$. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Additionally we have estimated the quadrupolar components of the anisotropy: they are not statistically significant. We discuss the results in the context of the predictions from different models for the distribution of ultrahigh-energy sources and cosmic magnetic fields., Comment: Published version, 16 pages, 7 figures, 8 tables
Published: 2018
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36. Understanding AGB evolution in Galactic bulge stars from high-resolution infrared spectroscopy

Author: Mathias Schultheis, S. Uttenthaler, Peter R. Wood, Nils Ryde, J. A. D. L. Blommaert, Thomas Lebzelter, Bernhard Aringer, Physics, Astrophysics, and Astronomy and Astrophysics Research Group
Subjects: 010504 meteorology & atmospheric sciences, Metallicity, K-type main-sequence star, FOS: Physical sciences, stars: AGB and post-AGB, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Galaxy: bulge, Bulge, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Asymptotic giant branch, stars: evolution, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Physics, Spiral galaxy, stars: late-type, Astronomy, Astronomy and Astrophysics, Galaxy, Radial velocity, Stars, Astrophysics - Solar and Stellar Astrophysics, 13. Climate action, Space and Planetary Science, Astrophysics::Earth and Planetary Astrophysics
Abstract: An analysis of high-resolution near-infrared spectra of a sample of 45 asymptotic giant branch (AGB) stars towards the Galactic bulge is presented. The sample consists of two subsamples, a larger one in the inner and intermediate bulge, and a smaller one in the outer bulge. The data are analysed with the help of hydrostatic model atmospheres and spectral synthesis. We derive the radial velocity of all stars, and the atmospheric chemical mix ([Fe/H], C/O, $^{12}$C/$^{13}$C, Al, Si, Ti, and Y) where possible. Our ability to model the spectra is mainly limited by the (in)completeness of atomic and molecular line lists, at least for temperatures down to $T_{\rm eff}\approx3100$ K. We find that the subsample in the inner and intermediate bulge is quite homogeneous, with a slightly sub-solar mean metallicity and only few stars with super-solar metallicity, in agreement with previous studies of non-variable M-type giants in the bulge. All sample stars are oxygen-rich, C/O$, Comment: 21 pages, 13 figures, 6 tables (incl. appendix), years of work, published in MNRAS
Published: 2015
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37. A first search for cosmogenic neutrinos with the ARIANNA Hexagonal Radio Array

Author: D. Z. Besson, R. G. Bose, G. Yodh, A. Samanta, Ulrik I. Uggerhøj, E. C. Berg, Stijn Buitink, Kenneth L. Ratzlaff, J. H. Buckley, Jordan C. Hanson, G. Binder, K. Dookayka, J. Walker, S. Euler, Hans Niederhausen, Brian Rauch, L. Gerhardt, Leif Gustafsson, Steven W. Barwick, G. E. Simburger, C. Reed, W. R. Binns, T. Duffin, M. H. Israel, S. R. Klein, C. Persichelli, P. F. Dowkontt, D. J. Boersma, Stuart A. Kleinfelder, V. Bugaev, Allan Hallgren, M. A. Olevitch, R. Young, M. Roumi, D. L. Braun, J. Tatar, T. Stezelberger, J. Kiryluk, Physics, and Astronomy and Astrophysics Research Group
Subjects: Physics::Instrumentation and Detectors, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Antartica, Flux, FOS: Physical sciences, Astrophysics, Atomic, ARIANNA Experiment, Nuclear physics, Particle and Plasma Physics, Neutrino, Cosmogenic, Nuclear, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, Physics, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), Detector, Molecular, Astronomy and Astrophysics, Solar neutrino problem, GZK, Radio, Nuclear & Particles Physics, radio, Neutrino detector, High energy, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Antarctica, High Energy Physics::Experiment, Radio frequency, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, physics, Astronomical and Space Sciences, astro-ph.IM
Abstract: The ARIANNA experiment seeks to observe the diffuse flux of neutrinos in the 10^8 - 10^10 GeV energy range using a grid of radio detectors at the surface of the Ross Ice Shelf of Antarctica. The detector measures the coherent Cherenkov radiation produced at radio frequencies, from about 100 MHz to 1 GHz, by charged particle showers generated by neutrino interactions in the ice. The ARIANNA Hexagonal Radio Array (HRA) is being constructed as a prototype for the full array. During the 2013-14 austral summer, three HRA stations collected radio data which was wirelessly transmitted off site in nearly real-time. The performance of these stations is described and a simple analysis to search for neutrino signals is presented. The analysis employs a set of three cuts that reject background triggers while preserving 90% of simulated cosmogenic neutrino triggers. No neutrino candidates are found in the data and a model-independent 90% confidence level Neyman upper limit is placed on the all flavor neutrino+antineutrino flux in a sliding decade-wide energy bin. The limit reaches a minimum of 1.9x10^-23 GeV^-1 cm^-2 s^-1 sr^-1 in the 10^8.5 - 10^9.5 GeV energy bin. Simulations of the performance of the full detector are also described. The sensitivity of the full ARIANNA experiment is presented and compared with current neutrino flux models., 22 pages, 22 figures. Published in Astroparticle Physics
Published: 2015
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38. Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves

Author: Maarten Baes, F. Allaert, G. Gentile, Astrophysics, Physics, and Astronomy and Astrophysics Research Group
Subjects: DWARF GALAXIES, DISC GALAXIES, Dark matter, galaxies: halos, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Disc galaxy, 01 natural sciences, dark matter, SURFACE BRIGHTNESS GALAXIES, SPHERICAL GALAXIES, kinematics and dynamics [galaxies], 0103 physical sciences, Galaxies: Evolution, 010303 astronomy & astrophysics, evolution [galaxies], Galaxy rotation curve, galaxies: kinematics and dynamics, Astrophysics::Galaxy Astrophysics, MASS-DISTRIBUTION, Dwarf galaxy, Physics, Spiral galaxy, 010308 nuclear & particles physics, GALACTIC HALOS, Astronomy and Astrophysics, PROFILES, Astrophysics - Astrophysics of Galaxies, Galaxy, halos [galaxies], Dark matter halo, Physics and Astronomy, Space and Planetary Science, Halo, STELLAR MASS, SPIRAL GALAXIES, CUSPS
Abstract: Recent cosmological hydrodynamical simulations suggest that baryonic processes, and in particular supernova feedback after bursts of star formation, can alter the structure of dark matter haloes and transform primordial cusps into shallower cores. To assess whether this mechanism offers a solution to the cusp-core controversy, simulated haloes must be compared to real dark matter haloes inferred from galaxy rotation curves. For this purpose, two new dark matter density profiles were recently derived from simulations of galaxies in complementary mass ranges: the DC14 halo ($10^{10} < M_{\text{halo}}/M_{\odot} < 8 \times 10^{11}$) and the coreNFW halo ($10^{7} < M_{\text{halo}}/M_{\odot} < 10^{9}$). Both models have individually been found to give good fits to observed rotation curves. For the DC14 model, however, the agreement of the predicted halo properties with cosmological scaling relations was confirmed by one study, but strongly refuted by another. A next question is whether the two models converge to the same solution in the mass range where both should be appropriate. To investigate this, we tested the DC14 and cNFW halo models on the rotation curves of a selection of galaxies with halo masses in the range $4 \times 10^{9}$ - $7 \times 10^{10}$ $M_{\odot}$. We further applied the DC14 model to a set of rotation curves at higher halo masses, up to $9 \times 10^{11}$ $M_{\odot}$, to verify the agreement with the cosmological scaling relations. We find that both models are generally able to reproduce the observed rotation curves, in line with earlier results, and the predicted dark matter haloes are consistent with the cosmological $c-M_{\text{halo}}$ and $M_{*}-M_{\text{halo}}$ relations. The DC14 and cNFW models are also in fairly good agreement with each other, even though DC14 tends to predict slightly less extended cores and somewhat more concentrated haloes than cNFW., Comment: 19 pages, 12 figures, accepted for publication in A&A
Published: 2017

39. HALOGAS Observations of NGC 4559: Anomalous and Extraplanar H I and its Relation to Star Formation

Author: Rene A. M. Walterbos, Maria T. Patterson, Filippo Fraternali, Paolo Serra, G. Gentile, George Heald, Gyula I. G. Józsa, Richard J. Rand, Carlos J. Vargas, Astronomy, Vargas, Carlos J., Heald, George, Walterbos, René A. M., Fraternali, Filippo, Patterson, Maria T., Rand, Richard J., Józsa, Gyula I. G., Gentile, Gianfranco, Serra, Paolo, Physics, and Astronomy and Astrophysics Research Group
Subjects: galaxies: spiral, DWARF GALAXIES, Milky Way, galaxies: halos, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, EXTRA-PLANAR GAS, 01 natural sciences, Spectral line, DIFFUSE IONIZED-GAS, 0103 physical sciences, GASEOUS HALOS, NEARBY GALAXIES, galaxies: halos, galaxies: ISM, galaxies: spiral, HIGH-VELOCITY CLOUDS, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Dwarf galaxy, Physics, Spiral galaxy, 010308 nuclear & particles physics, Star formation, Astronomy, Astronomy and Astrophysics, Scale height, DISK GALAXIES, Galaxy, NEUTRAL HYDROGEN, Stars, Space and Planetary Science, MILKY-WAY, SPIRAL GALAXIES, galaxies: ISM
Abstract: We use new deep 21 cm H i observations of the moderately inclined galaxy NGC 4559 in the HALOGAS survey to investigate the properties of extraplanar gas. We use TiRiFiC to construct simulated data cubes to match the H i observations. We find that a thick-disk component of scale height ∼2 kpc, characterized by a negative vertical gradient in its rotation velocity (lag) of ∼13 ± 5 km s −1 kpc −1 is an adequate fit to extraplanar gas features. The tilted ring models also present evidence for a decrease in the magnitude of the lag outside R 25 , and a radial inflow of ∼10 km s −1 . We extracted lagging extraplanar gas through Gaussian velocity profile fitting. From both the 3D models and extraction analyses we conclude that ∼10%–20% of the total H i mass is extraplanar. Most of the extraplanar gas is spatially coincident with regions of star formation in spiral arms, as traced by H α and GALEX FUV images, so it is likely due to star formation processes driving a galactic fountain. We also find the signature of a filament of a kinematically “forbidden” H i feature, containing ∼1.4 × 10 6 M ⊙ of H i , and discuss its potential relationship to a nearby H i hole. We discover a previously undetected dwarf galaxy in H i located ∼0.°4 (∼58 kpc) from the center of NGC 4559, containing ∼4 × 10 5 M ⊙ . This dwarf has counterpart sources in SDSS with spectra typical of H ii regions, and we conclude that it is two merging blue compact dwarf galaxies.
Published: 2017
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40. Thunderstorm electric fields probed by extensive air showers through their polarized radio emission

Author: Olaf Scholten, Anna Nelles, Brian Hare, Tobias Winchen, Pim Schellart, Satyendra Thoudam, Ute Ebert, Casper Rutjes, J. E. Enriquez, S. ter Veen, Laura Rossetto, Pragati Mitra, T. N. G. Trinh, Arthur Corstanje, Jörg P. Rachen, Jörg R. Hörandel, Stijn Buitink, Katie Mulrey, Heino Falcke, Antonio Bonardi, Physics, Astronomy and Astrophysics Research Group, Faculty of Sciences and Bioengineering Sciences, Research unit Astroparticle Physics, and Elementary Processes in Gas Discharges
Subjects: Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Atmospheric sciences, 01 natural sciences, symbols.namesake, Electric field, 0103 physical sciences, Stokes parameters, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Circular polarization, Physics::Atmospheric and Oceanic Physics, Physics, 010308 nuclear & particles physics, LOFAR, COSMIC-RAYS, Computational physics, Transverse plane, 13. Climate action, symbols, Thunderstorm, RADIATION, ARRAY, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We observe a large fraction of circular polarization in radio emission from extensive air showers recorded during thunderstorms, much higher than in the emission from air showers measured during fair-weather circumstances. We show that the circular polarization of the air showers measured during thunderstorms can be explained by the change in the direction of the transverse current as a function of altitude induced by atmospheric electric fields. Thus by using the full set of Stokes parameters for these events, we obtain a good characterization of the electric fields in thunderclouds. We also measure a large horizontal component of the electric fields in the two events that we have analyzed.
Published: 2017
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41. A study of radio frequency spectrum emitted by high energy air showers with LOFAR

Author: Tobias Winchen, Antonio Bonardi, Sander ter Veen, Heino Falcke, Stijn Buitink, Katie Mulrey, Anna Nelles, Olaf Scholten, Pim Schellart, Arthur Corstanje, Laura Rossetto, Jörg P. Rachen, Jörg R. Hörandel, Gia Trinh, J. Emilio Enriquez, Satyendra Thoudam, Pragati Mitra, Physics, Astronomy and Astrophysics Research Group, Faculty of Sciences and Bioengineering Sciences, and Research unit Astroparticle Physics
Subjects: Physics, 010308 nuclear & particles physics, QC1-999, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Detector, Monte Carlo method, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics, LOFAR, Astrophysics::Cosmology and Extragalactic Astrophysics, Low frequency, Physics and Astronomy(all), 01 natural sciences, Radio spectrum, Computational physics, Radio telescope, 0103 physical sciences, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: The LOw Frequency ARray (LOFAR) is a multipurpose radio antenna array aimed to detect radio signals in the frequency range 10 - 240 MHz, covering a large surface in Northern Europe with a higher density in the Northern Netherlands. The detection of the radio signal emitted by extensive air showers allows to reconstruct the geometry of the observed cascade. Thus, several properties of primary particles (e.g. arrival direction, mass composition) can be inferred. We describe a study of several geometrical parameters of the radio signal emitted by extensive air showers propagating in the atmosphere, and their correlation with the observed radio frequency spectrum. In order to find the best parameters that describe the correlation between primary cosmic ray information and the emitted radio signal, a preliminary study on simulated events has been done. Monte Carlo simulations of radio signals have been produced by using the CoREAS code, a plug-in of the CORSIKA particle simulation code. The final aim of this study is to find a method to infer information of primary cosmic rays in an independent way from the well-established fluorescence and surface detector techniques, in view of affirming the radio detection technique as reliable method for the study of high energy cosmic rays.
Published: 2017

42. Interpretation of the cosmic-ray air shower signal in Askaryan radio detectors

Author: Nick van Eijndhoven, Aongus O'Murchadha, Krijn de Vries, Stijn Buitink, Olaf Scholten, Thomas Meures, Horandel, Jorg R., Lahmann, Robert, Scholten, Olaf, De Jong, Sijbrand, Nahnhauer, Rolf, Buitink, Stijn, Physics, Elementary Particle Physics, Astronomy and Astrophysics Research Group, and Research unit Astroparticle Physics
Subjects: Physics, 010308 nuclear & particles physics, QC1-999, Astrophysics::High Energy Astrophysical Phenomena, Detector, Cosmic ray, Généralités, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Physics and Astronomy(all), 01 natural sciences, Physics::Geophysics, Shower, Air shower, Transition radiation, Radio signal, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, 010306 general physics, Physics::Atmospheric and Oceanic Physics
Abstract: We discuss the radio emission from a cosmic-ray air shower propagating in air before it hits an air-ice boundary after which it completes its propagation inside the ice. The in-air emission, the in-ice emission, as well as the transition radiation from the shower crossing the boundary is considered. We discuss the interpretation of the radio signal observed by an in-ice observer., SCOPUS: cp.p, info:eu-repo/semantics/published
Published: 2017

43. The Herschel Exploitation of Local Galaxy Andromeda (HELGA)

Author: George J. Bendo, S. Verstocken, Sébastien Viaene, Antti Tamm, S. C. Madden, P. De Vis, Matthew Smith, Maarten Baes, Médéric Boquien, Elmo Tempel, Peter Camps, Joris Blommaert, L. Spinoglio, Maud Galametz, J. A. Fernández-Ontiveros, A. Cooray, Gianfranco Gentile, Alessandro Boselli, Jacopo Fritz, I. De Looze, Physics, Astronomy and Astrophysics Research Group, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), and Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
Subjects: Andromeda Galaxy, ISM [Infrared], FOS: Physical sciences, SPECTRAL ENERGY-DISTRIBUTIONS, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, TRANSFER SIMULATIONS, 01 natural sciences, Luminosity, Atmospheric radiative transfer codes, Bulge, 0103 physical sciences, ISM [Galaxies], STAR-FORMING GALAXIES, Radiative transfer, Astrophysics::Solar and Stellar Astrophysics, NEARBY GALAXIES, COLD DUST, EDGE-ON GALAXIES, individual: M31 [galaxies], 010303 astronomy & astrophysics, Dust, extinction, Astrophysics::Galaxy Astrophysics, SPITZER-SPACE-TELESCOPE, Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], extinction, 010308 nuclear & particles physics, Star formation, Astronomy and Astrophysics, SPIRAL GALAXY, Astrophysics - Astrophysics of Galaxies, FORMATION RATES, Galaxy, Interstellar medium, Physics and Astronomy, individual: M 31 [Galaxies], 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), fundamental parameters [Galaxies], galaxies: individual: M 31, galaxies: ISM, infrared: ISM, galaxies: fundamental parameters, dust, extinction, radiative transfer, MILKY-WAY, dust, Astrophysics::Earth and Planetary Astrophysics
Abstract: The radiation of stars heats dust grains in the diffuse interstellar medium and in star-forming regions in galaxies. Modelling this interaction provides information on dust in galaxies, a vital ingredient for their evolution. It is not straightforward to identify the stellar populations heating the dust, and to link attenuation to emission on a sub-galactic scale. Radiative transfer models are able to simulate this dust-starlight interaction in a realistic, three-dimensional setting. We investigate the dust heating mechanisms on a local and global galactic scale, using the Andromeda galaxy (M31) as our laboratory. We perform a series of panchromatic radiative transfer simulations of Andromeda with our code SKIRT. The high inclination angle of M31 complicates the 3D modelling and causes projection effects. However, the observed morphology and flux density are reproduced fairly well from UV to sub-millimeter wavelengths. Our model reveals a realistic attenuation curve, compatible with previous, observational estimates. We find that the dust in M31 is mainly (91 % of the absorbed luminosity) heated by the evolved stellar populations. The bright bulge produces a strong radiation field and induces non-local heating up to the main star-forming ring at 10 kpc. The relative contribution of unevolved stellar populations to the dust heating varies strongly with wavelength and with galactocentric distance.The dust heating fraction of unevolved stellar populations correlates strongly with NUV-r colour and specific star formation rate. These two related parameters are promising probes for the dust heating sources at a local scale., Comment: 16 pages + appendix, 13 figures, accepted for publication in A&A
Published: 2017
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44. The effect of the atmospheric refractive index on the radio signal of extensive air showers

Author: Stijn Buitink, Katie Mulrey, A. Nelles, Tobias Winchen, S. ter Veen, Jörg P. Rachen, Jörg R. Hörandel, Laura Rossetto, Pragati Mitra, Pim Schellart, Antonio Bonardi, Heino Falcke, Arthur Corstanje, Satyendra Thoudam, Gia Trinh, Olaf Scholten, Research unit Astroparticle Physics, Physics, Astronomy and Astrophysics Research Group, Faculty of Sciences and Bioengineering Sciences, and Elementary Particle Physics
Subjects: Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Atmospheric sciences, 01 natural sciences, 0103 physical sciences, Extensive air showers, Radio emission, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Cosmic rays, Zenith, Cherenkov radiation, High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, astro-ph.HE, Atmospheric pressure, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Humidity, Astronomy and Astrophysics, Atmospheric effects, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Refractive index, Radio wave, astro-ph.IM
Abstract: For the interpretation of measurements of radio emission from extensive air showers, an important systematic uncertainty arises from natural variations of the atmospheric refractive index $n$. At a given altitude, the refractivity $N=10^6\, (n-1)$ can have relative variations on the order of $10 \%$ depending on temperature, humidity, and air pressure. Typical corrections to be applied to $N$ are about $4\%$. Using CoREAS simulations of radio emission from air showers, we have evaluated the effect of varying $N$ on measurements of the depth of shower maximum $X_{\rm max}$. For an observation band of 30 to 80 MHz, a difference of $4 \%$ in refractivity gives rise to a systematic error in the inferred $X_{\rm max}$ between 3.5 and 11 $\mathrm{g/cm^2}$, for proton showers with zenith angles ranging from 15 to 50 degrees. At higher frequencies, from 120 to 250 MHz, the offset ranges from 10 to 22 $\mathrm{g/cm^2}$. These offsets were found to be proportional to the geometric distance to $X_{\rm max}$. We have compared the results to a simple model based on the Cherenkov angle. For the 120 to 250 MHz band, the model is in qualitative agreement with the simulations. In typical circumstances, we find a slight decrease in $X_{\rm max}$ compared to the default refractivity treatment in CoREAS. While this is within commonly treated systematic uncertainties, accounting for it explicitly improves the accuracy of $X_{\rm max}$ measurements., 13 pages, 5 figures. Accepted for publication in Astroparticle Physics
Published: 2017

45. Search for Cosmic Particles with the Moon and LOFAR

Author: T. N. G. Trinh, Olaf Scholten, S. ter Veen, Jörg P. Rachen, Jörg R. Hörandel, Laura Rossetto, Arthur Corstanje, Anna Nelles, Satyendra Thoudam, Pragati Mitra, Tobias Winchen, J. E. Enriquez, Katharine Mulrey, A. Bonardi, Heino Falcke, Pim Schellart, Stijn Buitink, Research unit Astroparticle Physics, Physics, Astronomy and Astrophysics Research Group, and Faculty of Sciences and Bioengineering Sciences
Subjects: Physics, COSMIC cancer database, 010308 nuclear & particles physics, QC1-999, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, LOFAR, Physics and Astronomy(all), 01 natural sciences, Radio telescope, 0103 physical sciences, Particle, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract: The low flux of the ultra-high energy cosmic rays (UHECR) at the highest energies provides a challenge to answer the long standing question about their origin and nature. A significant increase in the number of detected UHECR is expected to be achieved by employing Earth's moon as detector, and search for short radio pulses that are emitted when a particle interacts in the lunar rock. Observation of these short pulses with current and future radio telescopes also allows to search for the even lower fluxes of neutrinos with energies above $10^{22}$ eV, that are predicted in certain Grand-Unifying-Theories (GUTs), and e.g. models for super-heavy dark matter (SHDM). In this contribution we present the initial design for such a search with the LOFAR radio telescope., Comment: To be published in the Proceedings of the ARENA2016 conference, Groningen, The Netherlands
Published: 2017

46. Overview of lunar detection of ultra-high energy particles and new plans for the SKA

Author: Sander ter Veen, Rustam D. Dagkesamanskii, M. Mevius, Tobias Winchen, Ronald D. Ekers, R. L. Mutel, Heino Falcke, Justin D. Bray, Ralph Spencer, Stijn Buitink, Olaf Scholten, Jaime Alvarez-Muñiz, Ken Gayley, Tim Huege, C. W. James, Research unit Astroparticle Physics, Physics, and Astronomy and Astrophysics Research Group
Subjects: High energy, Astronomy, QC1-999, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Physics and Astronomy(all), 01 natural sciences, Radio telescope, 0103 physical sciences, ddc:530, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, COSMIC cancer database, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Square kilometre array, Particle, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The lunar technique is a method for maximising the collection area for ultra-high-energy (UHE) cosmic ray and neutrino searches. The method uses either ground-based radio telescopes or lunar orbiters to search for Askaryan emission from particles cascading near the lunar surface. While experiments using the technique have made important advances in the detection of nanosecond-scale pulses, only at the very highest energies has the lunar technique achieved competitive limits. This is expected to change with the advent of the Square Kilometre Array (SKA), the low-frequency component of which (SKA-low) is predicted to be able to detect an unprecedented number of UHE cosmic rays. In this contribution, the status of lunar particle detection is reviewed, with particular attention paid to outstanding theoretical questions, and the technical challenges of using a giant radio array to search for nanosecond pulses. The activities of SKA's High Energy Cosmic Particles Focus Group are described, as is a roadmap by which this group plans to incorporate this detection mode into SKA-low observations. Estimates for the sensitivity of SKA-low phases 1 and 2 to UHE particles are given, along with the achievable science goals with each stage. Prospects for near-future observations with other instruments are also described., 6 pages, 3 figures, presented at the 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2016), Groningen, The Netherlands
Published: 2017
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47. SLAC T-510: Radio emission from particle cascades in the presence of a magnetic field

Author: Katharine Mulrey, Physics, and Astronomy and Astrophysics Research Group
Subjects: Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Cosmic ray, Astrophysics, Radiation, Physics and Astronomy(all), 01 natural sciences, Computational physics, Magnetic field, Earth's magnetic field, Cascade, 0103 physical sciences, Cathode ray, Particle, Radio frequency, 010306 general physics
Abstract: Cosmic ray induced particle cascades radiate in radio frequencies in the Earth’s atmosphere. Geomagnetic and Askaryan emission provide an effective way to detect ultra-high energy cosmic rays. The SLAC T-510 experiment was the first to measure magnetically induced radiation from particle cascades in a controlled laboratory setting. An electron beam incident upon a dense dielectric target produced a particle cascade in the presence of a variable magnetic field. Antennas covering a band of 30-3000 MHz sampled RF emission in vertical and horizontal polarizations. Results from T-510 are compared to particle-level RF-emission simulations which are critical for reconstructing the energy and composition of detected ultra-high energy cosmic ray air showers. We discuss the experimental set up, the data processing, the systematic errors and the main results of the experiment, which we found in a good agreement with the simulations.
Published: 2017

48. Towards real-time cosmic-ray identification with the LOw Frequency ARay

Author: Anna Nelles, Antonio Bonardi, Brian Hare, Stijn Buitink, Katie Mulrey, Sander ter Veen, Jörg P. Rachen, Jörg R. Hörandel, Pragati Mitra, Satyendra Thoudam, Heino Falcke, Pim Schellart, Gia Trinh, Olaf Scholten, Laura Rossetto, Tobias Winchen, Arthur Corstanje, Astronomy and Astrophysics Research Group, Physics, and Faculty of Sciences and Bioengineering Sciences
Subjects: Physics, 010308 nuclear & particles physics, business.industry, QC1-999, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Limiting, LOFAR, Low frequency, 01 natural sciences, Particle detector, Identification (information), Optics, 0103 physical sciences, Recognition system, Antenna (radio), 010306 general physics, business
Abstract: The radio signals emitted by Extensive Air Showers have been successfully used for the last decade by LOFAR to reconstruct the properties of the primary cosmic rays. Since an effective real-time recognition system for the very short radio pulses is lacking, cosmic-ray acquisition is currently triggered by an external array of particle detector, called LORA, limiting the LOFAR collecting area to the area covered by LORA. A new algorithm for the real-time cosmic-ray detection has been developed for the LOFAR Low Band Antenna, which are sensitive between 10 and 90 MHz, and is here presented together with the latest results.
Published: 2019
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49. A new parametrization for the radio emission of air showers applied to LOFAR data

Author: Brian Hare, Arthur Corstanje, Antonio Bonardi, Pim Schellart, Pragati Mitra, Tobias Winchen, Jörg R. Hörandel, Heino Falcke, J. P. Rachen, T. N. G. Trinh, I. Plaisier, Satyendra Thoudam, S. ter Veen, Laura Rossetto, Anna Nelles, Stijn Buitink, Katie Mulrey, Olaf Scholten, S. J. De Jong, Astronomy and Astrophysics Research Group, Physics, and Faculty of Sciences and Bioengineering Sciences
Subjects: Physics, QC1-999, Astronomy, Computer Science::Information Retrieval, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, LOFAR, Mass composition, Computational physics, Earth's magnetic field, Primary (astronomy), Energy density, High Energy Physics, Parametrization, Energy (signal processing)
Abstract: The energy and mass composition of cosmic rays influence how the energy density of the radio emission of air showers is distributed on the ground. A precise description of the radio profiles can, therefore, be used to reconstruct the properties of the primary cosmic rays. Here, such a description is presented, using a separate treatment of the two radio-emission mechanisms, the geomagnetic effect and the charge excess effect. The model is parametrized as a function that depends only on the shower parameters, allowing for a precise reconstruction of the properties of the primary cosmic rays. This model is applied to cosmic-ray events measured with LOFAR and it is capable of reconstructing the properties of air showers correctly.
Published: 2019
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50. Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum

Author: S. Stanič, Denis Stanca, J. A.J. Matthews, Xavier Bertou, M. L. Díaz Castro, C. Porowski, Jakub Vicha, Francesca Zuccarello, Pedro Assis, R. Sato, Jose Chinellato, I. Jandt, Hermann-Josef Mathes, M. Ziolkowski, Denise Boncioli, Markus Risse, Muller, F. Canfora, J. Blazek, A. Tonachini, Antonio Bueno, M. Josebachuili, J.D. Sanabria Gomez, Eric Mayotte, A. C. Rovero, J. Biteau, P.F. Gómez Vitale, G. A. Anastasi, Kai Daumiller, Alberto Filevich, Peter Hansen, John Matthews, Christian Sarmiento-Cano, Gualberto Avila, W. Rodrigues de Carvalho, Marco Torri, Nicolás González, M. Gómez Berisso, R. C. Shellard, Leigui de Oliveira, Paul M. Mantsch, Diego Ravignani, J. R. Vázquez, P. Sanchez-Lucas, S. Vorobiov, Ingomar Allekotte, F. Sánchez, J. W. Cronin, Lorenzo Cazon, Peter Buchholz, R. Piegaia, I. Al Samarai, Ivo Nicolas Naranjo, Antonio Insolia, A. Aab, L. Caramete, Alina Mihaela Badescu, P. Heimann, Anderson Fauth, M. Zavrtanik, G. Marsella, R. Ramos-Pollant, Valerio Pirronello, G. Torralba Elipe, O. Ravel, P. van Bodegom, Angela V. Olinto, C. Di Giulio, S. Navas, I.M. Brancus, H. Glass, Marco Aglietta, Johannes Schumacher, Joshua A. Gordon, Bruno Daniel, Corinne Berat, R. Krause, Gaia Silli, A. Filipčič, Foteini Oikonomou, G. S. Varner, Alessio Gorgi, Fred Sarazin, H. Gemmeke, Lukas Nellen, M. I. Micheletti, L. A. S. Pereira, Maria Giller, J. J. Masías Meza, C. J. Todero Peixoto, A.E. Herve, Octavian Sima, Nataliia Borodai, D. Mockler, Manuel Platino, E.M. Holt, B. Wundheiler, A. Fuster, Q. Hasankiadeh, A. Saleh, Jeffrey Brack, J. F. Valdés Galicia, Olaf Scholten, Ioana Codrina Maris, I. De Mitri, Dieter Heck, Martin Urban, Hans Klages, H. Nožka, A. Chiavassa, Maria-Teresa Dova, M. R. Hampel, O. A. Taborda, Carlos Hojvat, Miroslav Palatka, A. Menshikov, Diego Harari, B. Gookin, S. Müller, Carola Dobrigkeit, M. Schauer, Humberto Ibarguen Salazar, Ricardo Vázquez, Antoine Letessier-Selvon, Ernesto Kemp, R. Legumina, P. H. Nguyen, Lawrence Wiencke, B. Sarkar, Sarka Wykes, C. Morello, E. M. Santos, G. Kukec Mezek, L. Molina-Bueno, M. Plum, Z. Zong, David Walz, Harald Schieler, O. Kambeitz, Jeffrey A. Johnsen, Sven Querchfeld, L. Perrone, Marco Giammarchi, Bruce R. Dawson, S. Quinn, Christian Glaser, J. Espadanal, Octavian Fratu, M. E. Bertaina, Alan Watson, Mihai Niculescu-Oglinzanu, Jonny Kleinfeller, Sergio Sciutto, L. Ochilo, M. Mallamaci, Alberto Segreto, Nicusor Arsene, D. Rogozin, J. de Oliveira, R.R. Prado, Alejandro Almela, P. Billoir, Tim Huege, Ana Martina Botti, Belén Andrada, J. Alvarez Castillo, G. C. Hill, R.C. dos Anjos, Lukas Middendorf, D. Pakk Selmi-Dei, F. Diogo, G. De Mauro, Henryk Wilczyński, Ralph Engel, J. J. Beatty, Norbert Kunka, D. Nitz, Günter Sigl, Silvia Mollerach, A. Śmiałkowski, Jörg R. Hörandel, Sutherland, Julian Rautenberg, Peter L. Biermann, F. Montanet, L. Niemietz, R. M. de Almeida, L. Tomankova, Christine Peters, Radomir Smida, Alberto Etchegoyen, John L. Harton, Peter Gorham, T. Paul, Paolo Privitera, Federico Suarez, A. Schulz, D. Reinert, A. López Casado, G. Matthiae, Andreas Weindl, D. Garcia-Pinto, Paul Sommers, Petr Schovanek, A. Di Matteo, Charles Timmermans, Luis A. Nunez, A. Blanco, P. Gouffon, N. Krohm, D. Torres Machado, L. Collica, P. Abreu, Brian Fick, Zbigniew Szadkowski, Alberto Daniel Supanitsky, D. Melo, Julien Aublin, A. Shadkam, M. J. Cooper, Miguel Mostafá, Mário Pimenta, Gregory R Snow, Pablo Ristori, Miroslav Pech, P. H. Kasper, Carlos Medina, M. Settimo, R. Ulrich, Rodrigo Pelayo, Stijn Buitink, E. Varela, D. Yelos, Andrej Dundovic, Marcus Niechciol, D. Martello, Luis A. Anchordoqui, Pavel Horvath, Danilo Zavrtanik, Lorenzo Caccianiga, V. M. Theodoro, Paula Gina Isar, F. Salesa Greus, G. Cataldi, Florian Gaté, Michael Unger, S. Jansen, Gero Müller, P. W. Younk, Sofia Andringa, Eun-Joo Ahn, P. Lautridou, C. Scarso, Elton J. G. Santos, Jiri Chudoba, Markus Roth, G. van Aar, Dusan Mandat, Q. Luce, V. de Souza, Alex Kääpä, Maria Rita Coluccia, A. van Vliet, Tanguy Pierog, R. Cester, Gustavo Medina-Tanco, Miroslav Hrabovský, L. del Peral, Jaroslaw Stasielak, Andreas Haungs, Matthias Kleifges, V. Verzi, Philipp Papenbreer, Colin Baus, Glennys R. Farrar, David Schmidt, J. Sorokin, K. H. Becker, H. Martinez, A. G. Mariazzi, A. Kuotb Awad, S. G. Blaess, C. Aramo, Sergio Dasso, Tristan Sudholz, Fausto Guarino, Juan Pallotta, R. López, B. Tome, C. Bleve, Alexandru Balaceanu, Petr Travnicek, Rodríguez-Frías, V. Scherini, Arnulfo Zepeda, Eduardo Quel, David Wittkowski, Laura Valore, Martín Miguel Freire, Thomas Harrison, Benoît Revenu, Germano Guedes, Danielle LaHurd, Olivier Deligny, P. Pieroni, Alan Coleman, T. Hebbeker, Vincenzo Rizi, Trent D. Grubb, G. Rodriguez Fernandez, Benedikt Zimmermann, Rúben Conceição, Toshihiro Fujii, M. Ambrosio, L. Lopes, J. Debatin, O. Martínez Bravo, Dariusz Glas, Juan Manuel Figueira, F. Arqueros, Alexandra Saftoiu, Tim Niggemann, Roberta Colalillo, J. Hulsman, B. Mitrica, Hernán Asorey, Francesco Strafella, Martina Bohacova, Patrick Allison, Heino Falcke, Jaime Alvarez-Muñiz, Alexandru Gherghel-Lascu, I. Lhenry-Yvon, A. Lucero, Juan Carlos D'Olivo, O. Wainberg, A. Valbuena-Delgado, Esteban Roulet, T. Suomijärvi, Karl-Heinz Kampert, Antonella Castellina, Piera Luisa Ghia, V. Novotny, Rossella Caruso, S. Mathys, M. Erfani, John Swain, Thomas Bretz, Ruben Squartini, I. A. Minaya, Corbin Covault, Peter Mazur, J. Pȩkala, Geraldina Golup, Alexander Grillo, S. J. De Jong, Katrin Link, Lino Miramonti, Ugo Giaccari, A. Tepe, J. R. T. de Mello Neto, M. Prouza, J. Rodriguez Rojo, Bianca Keilhauer, A. G. Chavez, F.G. Schröder, Enrique Zas, Fernando Contreras, Jesús Peña-Rodríguez, A. Dorofeev, L. Villaseñor, A. Bridgeman, S. J. Saffi, Markus Lauscher, F. Pedreira, J. Phuntsok, Raul Sarmento, M. Suarez Durán, H. Wahlberg, A. Parra, G. Parente, M. Trini, Johannes Schulz, Florian Lukas Briechle, A. Cancio, B. Caccianiga, Alexey Yushkov, Max Malacari, Lili Yang, Luca Latronico, Piotr Homola, Alex Tapia, Tobias Winchen, P. Lebrun, Karen S. Caballero-Mora, Martin Erdmann, Carla Bonifazi, Beatriz García, Roger W Clay, Stefano D'Amico, Jose A. Bellido, Daniel Kuempel, S. Sonntag, Carlos Escobar, Jaime Rosado, R.M. Kieckhafer, B. Vargas Cárdenas, I. Valiño, J. Neuser, Ivone F. M. Albuquerque, Ke Fang, I. Katkov, Richard Dallier, Gaetano Salina, A.M. van den Berg, Darko Veberič, Jan Ridky, Marc Weber, M. Buscemi, D. Nosek, Jan Ebr, Sergio Petrera, S. Messina, S. Coutu, Norberto Fazzini, Aab, A., Abreu, P., Aglietta, M., Ahn, E. J., Al Samarai, I., Albuquerque, I. F. M., Allekotte, I., Allison, P., Almela, A., Alvarez Castillo, J., Alvarez Muñiz, J., Ambrosio, M., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arqueros, F., Arsene, N., Asorey, H., Assis, P., Aublin, J., Avila, G., Badescu, A. M., Balaceanu, A., Baus, C., Beatty, J. J., Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Billoir, P., Biteau, J., Blaess, S. G., Blanco, A., Blazek, J., Bleve, Carla, Boháčová, M., Boncioli, D., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Brancus, I., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero Mora, K. S., Caccianiga, B., Caccianiga, L., Cancio, A., Canfora, F., Caramete, L., Caruso, R., Castellina, A., Cataldi, G., Cazon, L., Cester, R., Chavez, A. G., Chiavassa, A., Chinellato, J. A., Chudoba, J., Clay, R. W., Colalillo, R., Coleman, A., Collica, L., Coluccia, MARIA RITA, Conceição, R., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Cronin, J., Dallier, R., D'Amico, Stefano, Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., de Almeida, R. M., de Jong, S. J., De Mauro, G., de Mello Neto, J. R. T., DE MITRI, Ivan, de Oliveira, J., de Souza, V., Debatin, J., del Peral, L., Deligny, O., Di Giulio, C., Di Matteo, A., Díaz Castro, M. L., Diogo, F., Dobrigkeit, C., D'Olivo, J. C., Dorofeev, A., dos Anjos, R. C., Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Falcke, H., Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Fick, B., Figueira, J. M., Filevich, A., Filipčič, A., Fratu, O., Freire, M. M., Fujii, T., Fuster, A., García, B., Garcia Pinto, D., Gaté, F., Gemmeke, H., Gherghel Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Głas, D., Glaser, C., Glass, H., Golup, G., Gómez Berisso, M., Gómez Vitale, P. F., González, N., Gookin, B., Gordon, J., Gorgi, A., Gorham, P., Gouffon, P., Grillo, A. F., Grubb, T. D., Guarino, F., Guedes, G. P., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harton, J. L., Hasankiadeh, Q., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hill, G. C., Hojvat, C., Holt, E., Homola, P., Hörandel, J. R., Horvath, P., Hrabovský, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Jansen, S., Johnsen, J. A., Josebachuili, M., Kääpä, A., Kambeitz, O., Kampert, K. H., Kasper, P., Katkov, I., Keilhauer, B., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Kukec Mezek, G., Kunka, N., Kuotb Awad, A., Lahurd, D., Latronico, L., Lauscher, M., Lautridou, P., Lebrun, P., Legumina, R., Leigui de Oliveira, M. A., Letessier Selvon, A., Lhenry Yvon, I., Link, K., Lopes, L., López, R., López Casado, A., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariş, I. C., Marsella, Giovanni, Martello, Daniele, Martinez, H., Martínez Bravo, O., Masías Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthews, J. A. J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina, C., Medina Tanco, G., Melo, D., Menshikov, A., Messina, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Mockler, D., Molina Bueno, L., Mollerach, S., Montanet, F., Morello, C., Mostafá, M., Müller, G., Muller, M. A., Müller, S., Naranjo, I., Navas, S., Nellen, L., Neuser, J., Nguyen, P. H., Niculescu Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Nožka, H., Núñez, L. A., Ochilo, L., Oikonomou, F., Olinto, A., Pakk Selmi Dei, D., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pękala, J., Pelayo, R., Peña Rodriguez, J., Pereira, L. A. S., Perrone, Lorenzo, Peters, C., Petrera, S., Phuntsok, J., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Quel, E. J., Querchfeld, S., Quinn, S., Ramos Pollant, R., Rautenberg, J., Ravel, O., Ravignani, D., Reinert, D., Revenu, B., Ridky, J., Risse, M., Ristori, P., Rizi, V., Rodrigues de Carvalho, W., Rodriguez Fernandez, G., Rodriguez Rojo, J., Rodríguez Frías, M. D., Rogozin, D., Rosado, J., Roth, M., Roulet, E., Rovero, A. C., Saffi, S. J., Saftoiu, A., Salazar, H., Saleh, A., Salesa Greus, F., Salina, G., Sanabria Gomez, J. D., Sánchez, F., Sanchez Lucas, P., Santos, E. M., Santos, E., Sarazin, F., Sarkar, B., Sarmento, R., Sarmiento Cano, C., Sato, R., Scarso, C., Schauer, M., Scherini, Viviana, Schieler, H., Schmidt, D., Scholten, O., Schovánek, P., Schröder, F. G., Schulz, A., Schulz, J., Schumacher, J., Sciutto, S. J., Segreto, A., Settimo, Mariangela, Shadkam, A., Shellard, R. C., Sigl, G., Silli, G., Sima, O., Śmiałkowski, A., Šmída, R., Snow, G. R., Sommers, P., Sonntag, S., Sorokin, J., Squartini, R., Stanca, D., Stanič, S., Stasielak, J., Strafella, Francesco, Suarez, F., Suarez Durán, M., Sudholz, T., Suomijärvi, T., Supanitsky, A. D., Sutherland, M. S., Swain, J., Szadkowski, Z., Taborda, O. A., Tapia, A., Tepe, A., Theodoro, V. M., Timmermans, C., Todero Peixoto, C. J., Tomankova, L., Tomé, B., Tonachini, A., Torralba Elipe, G., Torres Machado, D., Torri, M., Travnicek, P., Trini, M., Ulrich, R., Unger, M., Urban, M., Valbuena Delgado, A., Valdés Galicia, J. F., Valiño, I., Valore, L., van Aar, G., van Bodegom, P., van den Berg, A. M., van Vliet, A., Varela, E., Vargas Cárdenas, B., Varner, G., Vázquez, J. R., Vázquez, R. A., Veberič, D., Verzi, V., Vicha, J., Villaseñor, L., Vorobiov, S., Wahlberg, H., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weindl, A., Wiencke, L., Wilczyński, H., Winchen, T., Wittkowski, D., Wundheiler, B., Wykes, S., Yang, L., Yelos, D., Younk, P., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zepeda, A., Zimmermann, B., Ziolkowski, M., Zong, Z., Zuccarello, F., Bleve, C., Colalillo, Roberta, Coluccia, M. R., D'Amico, S., De Mitri, I., Guarino, Fausto, Marsella, G., Martello, D., Pȩkala, J., Perrone, L., Scherini, V., Settimo, M., Strafella, F., Valore, Laura, Physics, Astronomy and Astrophysics Research Group, Elementary Particle Physics, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), and Pierre Auger Collaboration
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Nuclear and High Energy Physics, Proton, Pierre Auger Observatory, Cosmic Rays, Mass Composition, Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, Cosmic ray, Ankle, Cosmic rays, Mass composition, Astrophysics, 01 natural sciences, Auger, Observatory, 0103 physical sciences, ddc:530, High Energy Physics, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Cherenkov radiation, Ciencias Exactas, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Range (particle radiation), 010308 nuclear & particles physics, OBSERVATÓRIOS, Astrophysics::Instrumentation and Methods for Astrophysics, Física, lcsh:QC1-999, Physique atomique et nucléaire, Experimental High Energy Physics, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, lcsh:Physics
Abstract: We report a first measurement for ultrahigh energy cosmic rays of the correlation between the depth of shower maximum and the signal in the water Cherenkov stations of air-showers registered simultaneously by the fluorescence and the surface detectors of the Pierre Auger Observatory. Such a correlation measurement is a unique feature of a hybrid air-shower observatory with sensitivity to both the electromagnetic and muonic components. It allows an accurate determination of the spread of primary masses in the cosmic-ray flux. Up till now, constraints on the spread of primary masses have been dominated by systematic uncertainties. The present correlation measurement is not affected by systematics in the measurement of the depth of shower maximum or the signal in the water Cherenkov stations. The analysis relies on general characteristics of air showers and is thus robust also with respect to uncertainties in hadronic event generators. The observed correlation in the energy range around the ‘ankle’ at lg⁡(E/eV)=18.5–19.0 differs significantly from expectations for pure primary cosmic-ray compositions. A light composition made up of proton and helium only is equally inconsistent with observations. The data are explained well by a mixed composition including nuclei with mass A>4. Scenarios such as the proton dip model, with almost pure compositions, are thus disfavored as the sole explanation of the ultrahigh-energy cosmic-ray flux at Earth., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2016
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