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Your search keyword '"Felis, I"' showing total 6 results
Start Over Author "Felis, I" Publisher escholarship, university of california
6 results on '"Felis, I"'

1. Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Author

Albert, A, André, M, Anghinolfi, M, Ardid, M, Aubert, J-J, Aublin, J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Boumaaza, J, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, Distefano, C, Di Palma, I, Domi, A, Donà, R, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Khayati, N El, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fermani, P, Ferrara, G, Fusco, L, Gay, P, Glotin, H, Grégoire, T, Ruiz, R Gracia, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Maggi, G, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nuñez, A, Organokov, M, and Păvălaş, GE

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, gravitational waves, neutrinos, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.

Published
2019

2. Joint Constraints on Galactic Diffuse Neutrino Emission from the ANTARES and IceCube Neutrino Telescopes

Author

Albert, A, André, M, Anghinolfi, M, Ardid, M, Aubert, JJ, Aublin, J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Boumaaza, J, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chabab, M, El Moursli, RC, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Colomer, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, Distefano, C, Palma, ID, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, IE, Khayati, NE, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fermani, P, Ferrara, G, Fusco, L, Gay, P, Glotin, H, Grégoire, T, Ruiz, RG, Graf, K, Hallmann, S, Haren, HV, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, Jong, MD, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Khan-Chowdhury, NR, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Levi, G, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Nuñez, A, Organokov, M, Pǎvǎlaş, GE, and Pellegrino, C

Subjects
astro-ph.HE, Astronomy & Astrophysics, Astronomical and Space Sciences
Abstract

The existence of diffuse Galactic neutrino production is expected from cosmic-ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offering the opportunity to test the products of Galactic cosmic-ray interactions up to energies of hundreds of TeV. Here we present a search for this production using ten years of Astronomy with a Neutrino Telescope and Abyss environmental RESearch (ANTARES) track and shower data, as well as seven years of IceCube track data. The data are combined into a joint likelihood test for neutrino emission according to the KRAg model assuming a 5 PeV per nucleon Galactic cosmic-ray cutoff. No significant excess is found. As a consequence, the limits presented in this Letter start constraining the model parameter space for Galactic cosmic-ray production and transport.

Published
2018

3. Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Author

Albert, A, André, M, Anghinolfi, M, Ardid, M, Aubert, J-J, Aublin, J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, MC, Brânzaş, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Moursli, R Cherkaoui El, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Díaz, AF, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Khayati, N El, Elsässer, D, Enzenhöfer, A, Ettahiri, A, Fassi, F, Felis, I, Fusco, LA, Gay, P, Giordano, V, Glotin, H, Grégoire, T, Ruiz, R Gracia, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Illuminati, G, James, CW, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Kießling, D, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Organokov, M, Păvălaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, and Pradier, T

Subjects
Nuclear and Plasma Physics, Astronomical Sciences, Physical Sciences, gamma-ray burst: general, gravitational waves, neutrinos, astro-ph.HE, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Space sciences
Abstract

The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merger of this binary was also recorded by the Fermi Gamma-ray Burst Monitor (Fermi-GBM), and the Anti-Coincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory (INTEGRAL), indicating particle acceleration by the source. The precise location of the event was determined by optical detections of emission following the merger. We searched for high-energy neutrinos from the merger in the GeV-EeV energy range using the Antares, IceCube, and Pierre Auger Observatories. No neutrinos directionally coincident with the source were detected within ± 500 s around the merger time. Additionally, no MeV neutrino burst signal was detected coincident with the merger. We further carried out an extended search in the direction of the source for high-energy neutrinos within the 14 day period following the merger, but found no evidence of emission. We used these results to probe dissipation mechanisms in relativistic outflows driven by the binary neutron star merger. The non-detection is consistent with model predictions of short GRBs observed at a large off-axis angle.

Published
2017

4. Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

Author

Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, J-J, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, Bojaddaini, I El, Elsässer, D, Enzenhöfer, A, Felis, I, Fusco, LA, Galatà, S, Gay, P, Giordano, V, Glotin, H, Grégoire, T, Ruiz, R Gracia, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, Illuminati, G, James, CW, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Kießling, D, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mathieu, A, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Nezri, E, Păvălaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Quinn, L, Racca, C, Riccobene, G, Sánchez-Losa, A, Saldaña, M, Salvadori, I, and Samtleben, DFE

Subjects
astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission from GW151226, adopting the GW event's 3D localization, to less than 2×1051-2×1054 erg.

Published
2017

5. High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube

Author

Adrián-Martínez, S, Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, JJ, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, Elsässer, D, Enzenhöfer, A, Fehn, K, Felis, I, Fusco, LA, Galatà, S, Gay, P, Geißelsöder, S, Geyer, K, Giordano, V, Gleixner, A, Glotin, H, Gracia-Ruiz, R, Graf, K, Hallmann, S, Van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, Illuminati, G, James, CW, De Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Kießling, D, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefèvre, D, Leonora, E, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mathieu, A, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, PǍvǍlaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Roensch, K, Saldaña, M, Samtleben, DFE, Sánchez-Losa, A, and Sanguineti, M

Subjects
astro-ph.HE
Abstract

We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and Antares neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within ±500 s of the gravitational wave event, the number of neutrino candidates detected by IceCube and Antares were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.

Published
2016

6. THE FIRST COMBINED SEARCH FOR NEUTRINO POINT-SOURCES IN THE SOUTHERN HEMISPHERE WITH THE ANTARES AND ICECUBE NEUTRINO TELESCOPES

Author

Adrián-Martínez, S, Albert, A, André, M, Anton, G, Ardid, M, Aubert, J-J, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Chiarusi, T, Circella, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Dekeyser, I, Deschamps, A, De Bonis, G, Distefano, C, Donzaud, C, Dornic, D, Drouhin, D, Dumas, A, Eberl, T, Elsässer, D, Enzenhöfer, A, Fehn, K, Felis, I, Fermani, P, Folger, F, Fusco, LA, Galatà, S, Gay, P, Geißelsöder, S, Geyer, K, Giordano, V, Gleixner, A, Gracia-Ruiz, R, Graf, K, Hallmann, S, van Haren, H, Heijboer, AJ, Hello, Y, Hernández-Rey, JJ, Hößl, J, Hofestädt, J, Hugon, C, James, CW, de Jong, M, Kadler, M, Kalekin, O, Katz, U, Kießling, D, Kooijman, P, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lahmann, R, Lefèvre, D, Leonora, E, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martínez-Mora, JA, Mathieu, A, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, Păvălaş, GE, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Racca, C, Riccobene, G, Richter, R, Roensch, K, Saldaña, M, Samtleben, DFE, Sánchez-Losa, A, Sanguineti, M, Sapienza, P, Schmid, J, Schnabel, J, and Schüssler, F

Subjects
astroparticle physics, neutrinos, hep-ex, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We present the results of searches for point-like sources of neutrinos based on the first combined analysis of data from both the ANTARES and IceCube neutrino telescopes. The combination of both detectors, which differ in size and location, forms a window in the southern sky where the sensitivity to point sources improves by up to a factor of 2 compared with individual analyses. Using data recorded by ANTARES from 2007 to 2012, and by IceCube from 2008 to 2011, we search for sources of neutrino emission both across the southern sky and from a preselected list of candidate objects. No significant excess over background has been found in these searches, and flux upper limits for the candidate sources are presented for E -2.5 and E -2 power-law spectra with different energy cut-offs.

Published
2016

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