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Your search keyword '"Calvo, M."' showing total 40 results
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40 results on '"Calvo, M."'

1. The XXL Survey

Author

Adam, R., primary, Ricci, M., additional, Eckert, D., additional, Ade, P., additional, Ajeddig, H., additional, Altieri, B., additional, André, P., additional, Artis, E., additional, Aussel, H., additional, Beelen, A., additional, Benoist, C., additional, Benoît, A., additional, Berta, S., additional, Bing, L., additional, Birkinshaw, M., additional, Bourrion, O., additional, Boutigny, D., additional, Bremer, M., additional, Calvo, M., additional, Cappi, A., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Faccioli, L., additional, Ferrari, C., additional, Gastaldello, F., additional, Giles, P., additional, Gomez, A., additional, Goupy, J., additional, Hahn, O., additional, Hanser, C., additional, Horellou, C., additional, Kéruzoré, F., additional, Koulouridis, E., additional, Kramer, C., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Madden, S., additional, Maughan, B., additional, Maurogordato, S., additional, Maury, A., additional, Mauskopf, P., additional, Monfardini, A., additional, Muñoz-Echeverría, M., additional, Pacaud, F., additional, Perotto, L., additional, Pierre, M., additional, Pisano, G., additional, Pompei, E., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Sereno, M., additional, Schuster, K., additional, Sievers, A., additional, Tintoré Vidal, G., additional, Tucker, C., additional, and Zylka, R., additional

Published
2024
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2. Faint mm NIKA2 dusty star-forming galaxies: Finding the high-redshift population

Author

Bing, L.-J., primary, Beelen, A., additional, Lagache, G., additional, Adam, R., additional, Ade, P., additional, Ajeddig, H., additional, André, P., additional, Artis, E., additional, Aussel, H., additional, Benoît, A., additional, Berta, S., additional, Béthermin, M., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Gomez, A., additional, Goupy, J., additional, Kéruzoré, F., additional, Kramer, C., additional, Ladjelate, B., additional, Leclercq, S., additional, Liu, D.-Z., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Maury, A., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Muñoz-Echeverría, M., additional, Neri, R., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A. J., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Shu, S., additional, Sievers, A., additional, Tucker, C., additional, Xiao, M.-Y., additional, and Zylka, R., additional

Published
2024
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3. The stratification of ISM properties in the edge-on galaxy NGC 891 revealed by NIKA2

Author

Katsioli, S., primary, Xilouris, E. M., additional, Kramer, C., additional, Adam, R., additional, Ade, P., additional, Ajeddig, H., additional, André, P., additional, Artis, E., additional, Aussel, H., additional, Baes, M., additional, Beelen, A., additional, Benoît, A., additional, Berta, S., additional, Bing, L., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Clark, C. J. R., additional, De Looze, I., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Ejlali, G., additional, Galametz, M., additional, Galliano, F., additional, Gomez, A., additional, Goupy, J., additional, Hanser, C., additional, Hughes, A., additional, Jones, A. P., additional, Kéruzoré, F., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J.-F., additional, Madden, S. C., additional, Maury, A., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Muñoz-Echeverría, M., additional, Nersesian, A., additional, Pantoni, L., additional, Paradis, D., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A. J., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Smith, M. W. L., additional, Tedros, J., additional, Tabatabaei, F., additional, Tucker, C., additional, Ysard, N., additional, and Zylka, R., additional

Published
2023
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4. NIKA2 Cosmological Legacy Survey

Author

Bing, L., primary, Béthermin, M., additional, Lagache, G., additional, Adam, R., additional, Ade, P., additional, Ajeddig, H., additional, André, P., additional, Artis, E., additional, Aussel, H., additional, Beelen, A., additional, Benoît, A., additional, Berta, S., additional, Billot, N., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Elbaz, D., additional, Gkogkou, A., additional, Gomez, A., additional, Goupy, J., additional, Hanser, C., additional, Kéruzoré, F., additional, Kramer, C., additional, Ladjelate, B., additional, Liu, D., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Lustig, P., additional, Macías-Pérez, J. F., additional, Maury, A., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Muñoz-Echeverría, M., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A. J., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Tucker, C., additional, and Zylka, R., additional

Published
2023
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5. CONCERTO: Extracting the power spectrum of the [CII] emission line

Author

Van Cuyck, M., primary, Ponthieu, N., additional, Lagache, G., additional, Beelen, A., additional, Béthermin, M., additional, Gkogkou, A., additional, Aravena, M., additional, Benoit, A., additional, Bounmy, J., additional, Calvo, M., additional, Catalano, A., additional, Désert, F. X., additional, Dupé, F.-X., additional, Fasano, A., additional, Ferrara, A., additional, Goupy, J., additional, Hoarau, C., additional, Hu, W., additional, Lambert, J.-C, additional, Macías-Pérez, J. F., additional, Marpaud, J., additional, Mellema, G., additional, Monfardini, A., additional, and Pallottini, A., additional

Published
2023
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7. Multi-probe analysis of the galaxy cluster CL J1226.9+3332

Author

Muñoz-Echeverría, M., primary, Macías-Pérez, J. F., additional, Pratt, G. W., additional, Adam, R., additional, Ade, P., additional, Ajeddig, H., additional, André, P., additional, Arnaud, M., additional, Artis, E., additional, Aussel, H., additional, Bartalucci, I., additional, Beelen, A., additional, Benoît, A., additional, Berta, S., additional, Bing, L., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Ferragamo, A., additional, Gomez, A., additional, Goupy, J., additional, Hanser, C., additional, Kéruzoré, F., additional, Kramer, C., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Maury, A., additional, Mauskopf, P., additional, Mayet, F., additional, Melin, J.-B., additional, Monfardini, A., additional, Paliwal, A., additional, Perotto, L., additional, Pisano, G., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A. J., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Shu, S., additional, Sievers, A., additional, Tucker, C., additional, and Yepes, G., additional

Published
2023
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8. CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 deg2 field and the impact of field-to-field variance

Author

Gkogkou, A., primary, Béthermin, M., additional, Lagache, G., additional, Van Cuyck, M., additional, Jullo, E., additional, Aravena, M., additional, Beelen, A., additional, Benoit, A., additional, Bounmy, J., additional, Calvo, M., additional, Catalano, A., additional, Cora, S., additional, Croton, D., additional, de la Torre, S., additional, Fasano, A., additional, Ferrara, A., additional, Goupy, J., additional, Hoarau, C., additional, Hu, W., additional, Ishiyama, T., additional, Knudsen, K. K., additional, Lambert, J.-C., additional, Macías-Pérez, J. F., additional, Marpaud, J., additional, Mellema, G., additional, Monfardini, A., additional, Pallottini, A., additional, Ponthieu, N., additional, Prada, F., additional, Roehlly, Y., additional, Vallini, L., additional, and Walter, F., additional

Published
2023
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9. CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping

Author

Béthermin, M., primary, Gkogkou, A., additional, Van Cuyck, M., additional, Lagache, G., additional, Beelen, A., additional, Aravena, M., additional, Benoit, A., additional, Bounmy, J., additional, Calvo, M., additional, Catalano, A., additional, de Batz de Trenquelleon, B., additional, De Breuck, C., additional, Fasano, A., additional, Ferrara, A., additional, Goupy, J., additional, Hoarau, C., additional, Horellou, C., additional, Hu, W., additional, Julia, A., additional, Knudsen, K., additional, Lambert, J.-C., additional, Macias-Perez, J., additional, Marpaud, J., additional, Monfardini, A., additional, Pallottini, A., additional, Ponthieu, N., additional, Roehlly, Y., additional, Vallini, L., additional, Walter, F., additional, and Weiss, A., additional

Published
2022
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10. Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera

Author

Lestrade, J.-F., primary, Désert, F.-X., additional, Lagache, G., additional, Adam, R., additional, Ade, P., additional, Ajeddig, H., additional, André, P., additional, Artis, E., additional, Aussel, H., additional, Beelen, A., additional, Benoît, A., additional, Berta, S., additional, Béthermin, M., additional, Bing, L., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coulais, A., additional, De Petris, M., additional, Doyle, S., additional, Driessen, E. F. C., additional, Gomez, A., additional, Goupy, J., additional, Kéruzoré, F., additional, Kramer, C., additional, Ladjelate, B., additional, Leclercq, S., additional, Macías-Pérez, J. F., additional, Maury, A., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Muñoz-Echeverría, M., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A. J., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Shu, S., additional, Sievers, A., additional, Tucker, C., additional, and Zylka, R., additional

Published
2022
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11. NIKA 150 GHz polarization observations of the Crab nebula and its spectral energy distribution (Corrigendum)

Author

Ritacco, A., primary, Macías-Pérez, J. F., additional, Ponthieu, N., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Aumont, J., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Bracco, A., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, D’Addabbo, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Mauskopf, P., additional, Mayet, F., additional, Maury, A., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Rebolo-Iglesias, M., additional, Revéret, V., additional, Rodriguez, L., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Siringo, G., additional, Thum, C., additional, Triqueneaux, S., additional, Tucker, C., additional, Wiesemeyer, H., additional, and Zylka, R., additional

Published
2022
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12. Development and application of metamaterial-based half-wave plates for the NIKA and NIKA2 polarimeters

Author

Pisano, G., primary, Ritacco, A., additional, Monfardini, A., additional, Tucker, C., additional, Ade, P. A. R., additional, Shitvov, A., additional, Benoit, A., additional, Calvo, M., additional, Catalano, A., additional, Goupy, J., additional, Leclercq, S., additional, Macias-Perez, J., additional, Andrianasolo, A., additional, and Ponthieu, N., additional

Published
2022
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13. Accurate sky signal reconstruction for ground-based spectroscopy with kinetic inductance detectors

Author

Fasano, A., primary, Macías-Pérez, J. F., additional, Benoit, A., additional, Aguiar, M., additional, Beelen, A., additional, Bideaud, A., additional, Bounmy, J., additional, Bourrion, O., additional, Bres, G., additional, Calvo, M., additional, Castro-Almazán, J. A., additional, Catalano, A., additional, de Bernardis, P., additional, De Petris, M., additional, de Taoro, A. P., additional, Fernández-Torreiro, M., additional, Garde, G., additional, Génova-Santos, R., additional, Gomez, A., additional, Gómez-Renasco, M. F., additional, Goupy, J., additional, Hoarau, C., additional, Hoyland, R., additional, Lagache, G., additional, Marpaud, J., additional, Marton, M., additional, Monfardini, A., additional, Peel, M. W., additional, Pisano, G., additional, Ponthieu, N., additional, Rebolo, R., additional, Roudier, S., additional, Rubiño-Martín, J. A., additional, Tourres, D., additional, Tucker, C., additional, and Vescovi, C., additional

Published
2021
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14. A wide field-of-view low-resolution spectrometer at APEX: Instrument design and science forecast

Author

The CONCERTO Collaboration, Ade, P., Aravena, M., Barria, E., Beelen, A., Benoit, A., B��thermin, M., Bounmy, J., Bourrion, O., Bres, G., De Breuck, C., Calvo, M., Cao, Y., Catalano, A., D��sert, F. -X., Dur��n, C. A, Fasano, A., Fenouillet, T., Garcia, J., Garde, G., Goupy, J., Groppi, C., Hoarau, C., Lagache, G., Lambert, J. -C., Leggeri, J. -P., Levy-Bertrand, F., Macias-Perez, J., Mani, H., Marpaud, J., Mauskopf, P., Monfardini, A., Pisano, G., Ponthieu, N., Prieur, L., Roni, S., Roudier, S., Tourres, D., Tucker, C., Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology [2020-....] (Grenoble INP [2020-....]), Université Grenoble Alpes [2020-....] (UGA [2020-....])-Université Grenoble Alpes [2020-....] (UGA [2020-....])-Centre National de la Recherche Scientifique (CNRS), 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), 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 [2020-....] (UGA [2020-....])-Institut polytechnique de Grenoble - Grenoble Institute of Technology [2020-....] (Grenoble INP [2020-....]), Université Grenoble Alpes [2020-....] (UGA [2020-....]), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble [2020-....] (OSUG [2020-....]), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes [2020-....] (UGA [2020-....])-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes [2020-....] (UGA [2020-....]), CONCERTO, Cryogénie (Cryo), 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)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (HELFA), 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), 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 ), Electronique (ElecLab), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Magnétisme et Supraconductivité (MagSup), The CONCERTO Collaboration, Cardiff University, Universidad Diego Portales [Santiago] (UDP), Cryogénie (NEEL - Cryo), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Hélium : du fondamental aux applications (NEEL - HELFA), Electronique (NEEL - ElecLab), European Southern Observatory (ESO), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, European Southern Observatory [Santiago] (ESO), Arizona State University [Tempe] (ASU), Magnétisme et Supraconductivité (NEEL - MagSup), and Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2020-....] (UGA [2020-....])-Institut polytechnique de Grenoble - Grenoble Institute of Technology [2020-....] (Grenoble INP [2020-....])

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Context (language use), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Cosmology, law.invention, Telescope, law, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Galaxy cluster, Astrophysics::Galaxy Astrophysics, instrumentation: spectrographs, Physics, Spectrometer, 010308 nuclear & particles physics, instrumentation: detectors, Intensity mapping, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, telescopes, Redshift, Galaxy, Space and Planetary Science, cosmology: observations, Cosmology: observations, Instrumentation: detectors, Instrumentation: spectrographs, Telescopes, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Characterise the large-scale structure in the Universe from present times to the high redshift epoch of reionisation is essential to constraining the cosmology, the history of star formation and reionisation, measuring the gas content of the Universe and obtaining a better understanding of the physical process that drive galaxy formation and evolution. Using the integrated emission from unresolved galaxies or gas clouds, line intensity mapping (LIM) provides a new observational window to measure the larger properties of structure. This very promising technique motivates the community to plan for LIM experiments. We describe the development of a large field-of-view instrument, named CONCERTO, operating in the range 130-310 GHz from the APEX 12-meters telescope. CONCERTO is a low-resolution spectrometer based on the Lumped Element Kinetic Inductance Detectors technology. Spectra are obtained using a fast Fourier Transform Spectrometer (FTS), coupled to a dilution cryostat with base temperature of 0.1K. Two 2 kilo-pixels arrays of LEKID are mounted inside the cryostat that also contains the cold optics and the front-end electronics. We present in detail the technological choices leading to the instrumental concept, together with the design and fabrication of the instrument and preliminary laboratory tests on the detectors. We also give our best estimates of CONCERTO sensitivity and give predictions for two of the main scientific goals of CONCERTO, i.e. a [CII]-intensity mapping survey and observations of galaxy clusters. We provide a detail description of the instrument design. Based on realistic comparisons with existing instruments developed by our group (NIKA, NIKA2, and KISS), and on laboratory detectors characterisation, we provide an estimate of CONCERTO sensitivity on sky. Finally, we describe in detail two out of the main science goals offered by CONCERTO at APEX., Comment: Accepted for publication in Astronomy and Astrophysics

Published
2020
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15. Exploiting NIKA2/XMM-Newtonimaging synergy for intermediate-mass high-zgalaxy clusters within the NIKA2 SZ large program

Author

Kéruzoré, F., primary, Mayet, F., additional, Pratt, G. W., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Andrianasolo, A., additional, Arnaud, M., additional, Aussel, H., additional, Bartalucci, I., additional, Beelen, A., additional, Benoît, A., additional, Berta, S., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Gomez, A., additional, Goupy, J., additional, Kramer, C., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Mauskopf, P., additional, Monfardini, A., additional, Perotto, L., additional, Pisano, G., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Shu, S., additional, Sievers, A., additional, and Tucker, C., additional

Published
2020
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16. The XXL Survey

Author

Ricci, M., primary, Adam, R., additional, Eckert, D., additional, Ade, P., additional, André, P., additional, Andrianasolo, A., additional, Altieri, B., additional, Aussel, H., additional, Beelen, A., additional, Benoist, C., additional, Benoît, A., additional, Berta, S., additional, Bideaud, A., additional, Birkinshaw, M., additional, Bourrion, O., additional, Boutigny, D., additional, Bremer, M., additional, Calvo, M., additional, Cappi, A., additional, Chiappetti, L., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Faccioli, L., additional, Ferrari, C., additional, Fotopoulou, S., additional, Gastaldello, F., additional, Giles, P., additional, Gomez, A., additional, Goupy, J., additional, Hahn, O., additional, Horellou, C., additional, Kéruzoré, F., additional, Koulouridis, E., additional, Kramer, C., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Maughan, B., additional, Maurogordato, S., additional, Mauskopf, P., additional, Monfardini, A., additional, Pacaud, F., additional, Perotto, L., additional, Pierre, M., additional, Pisano, G., additional, Pompei, E., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Sánchez Portal, M., additional, Schuster, K., additional, Sereno, M., additional, Shu, S., additional, Sievers, A., additional, Tucker, C., additional, and Umetsu, K., additional

Published
2020
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18. Detection of the magnetar XTE J1810−197 at 150 and 260 GHz with the NIKA2 kinetic inductance detector camera

Author

Torne, P., primary, Macías-Pérez, J., additional, Ladjelate, B., additional, Ritacco, A., additional, Sánchez-Portal, M., additional, Berta, S., additional, Paubert, G., additional, Calvo, M., additional, Desvignes, G., additional, Karuppusamy, R., additional, Navarro, S., additional, John, D., additional, Sánchez, S., additional, Peñalver, J., additional, Kramer, M., additional, and Schuster, K., additional

Published
2020
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19. Calibration and performance of the NIKA2 camera at the IRAM 30-m Telescope

Author

Perotto, L., primary, Ponthieu, N., additional, Macías-Pérez, J. F., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Andrianasolo, A., additional, Aussel, H., additional, Beelen, A., additional, Benoît, A., additional, Berta, S., additional, Bideaud, A., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Comis, B., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, García, P., additional, Gomez, A., additional, Goupy, J., additional, John, D., additional, Kéruzoré, F., additional, Kramer, C., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Maury, A., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Navarro, S., additional, Peñalver, J., additional, Pierfederici, F., additional, Pisano, G., additional, Revéret, V., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Shu, S., additional, Sievers, A., additional, Tucker, C., additional, and Zylka, R., additional

Published
2020
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20. NIKA 150 GHz polarization observations of the Crab nebula and its spectral energy distribution

Author

Ritacco, A., primary, Macías-Pérez, J. F., additional, Ponthieu, N., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Aumont, J., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Bracco, A., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, D’Addabbo, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Mauskopf, P., additional, Mayet, F., additional, Maury, A., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Rebolo-Iglesias, M., additional, Revéret, V., additional, Rodriguez, L., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Siringo, G., additional, Thum, C., additional, Triqueneaux, S., additional, Tucker, C., additional, Wiesemeyer, H., additional, and Zylka, R., additional

Published
2018
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21. A NIKA view of two star-forming infrared dark clouds: Dust emissivity variations and mass concentration

Author

Rigby, A. J., primary, Peretto, N., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Aussel, H., additional, Beelen, A., additional, Benoît, A., additional, Bracco, A., additional, Bideaud, A., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Clark, C. J. R., additional, Comis, B., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2018
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22. First Sunyaev–Zel’dovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate

Author

Ruppin, F., primary, Mayet, F., additional, Pratt, G.W., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Arnaud, M., additional, Aussel, H., additional, Bartalucci, I., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Comis, B., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Mauskopf, P., additional, Monfardini, A., additional, Perotto, L., additional, Pisano, G., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Schuster, K., additional, Sievers, A., additional, Tucker, C., additional, and Zylka, R., additional

Published
2018
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23. Substructure and merger detection in resolved NIKA Sunyaev-Zel’dovich images of distant clusters

Author

Adam, R., primary, Hahn, O., additional, Ruppin, F., additional, Ade, P., additional, André, P., additional, Arnaud, M., additional, Bartalucci, I., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, D’Addabbo, A., additional, Désert, F.-X., additional, Doyle, S., additional, Ferrari, C., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Martinez Aviles, G., additional, Martizzi, D., additional, Maurogordato, S., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Pratt, G. W., additional, Revéret, V., additional, Ricci, M., additional, Ritacco, A., additional, Rodriguez, L., additional, Romero, C., additional, Roussel, H., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, Wu, H.-Y., additional, and Zylka, R., additional

Published
2018
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24. A multi-instrument non-parametric reconstruction of the electron pressure profile in the galaxy cluster CLJ1226.9+3332

Author

Romero, C., primary, McWilliam, M., additional, Macías-Pérez, J.-F., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Aussel, H., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, de Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2018
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25. The NIKA2 large-field-of-view millimetre continuum camera for the 30 m IRAM telescope

Author

Adam, R., primary, Adane, A., additional, Ade, P. A. R., additional, André, P., additional, Andrianasolo, A., additional, Aussel, H., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Bracco, A., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Evans, R., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Leggeri, J.-P., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Mauskopf, P., additional, Mayet, F., additional, Maury, A., additional, Monfardini, A., additional, Navarro, S., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2018
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26. Mapping the hot gas temperature in galaxy clusters using X-ray and Sunyaev-Zel’dovich imaging

Author

Adam, R., primary, Arnaud, M., additional, Bartalucci, I., additional, Ade, P., additional, André, P., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourdin, H., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, D’Addabbo, A., additional, Désert, F.-X., additional, Doyle, S., additional, Ferrari, C., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Macías-Pérez, J.-F., additional, Maurogordato, S., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Pratt, G. W., additional, Revéret, V., additional, Ritacco, A., additional, Rodriguez, L., additional, Romero, C., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2017
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27. Probing changes of dust properties along a chain of solar-type prestellar and protostellar cores in Taurus with NIKA

Author

Bracco, A., primary, Palmeirim, P., additional, André, Ph., additional, Adam, R., additional, Ade, P., additional, Bacmann, A., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, D’Addabbo, A., additional, Désert, F.-X., additional, Didelon, P., additional, Doyle, S., additional, Goupy, J., additional, Könyves, V., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Macías-Pérez, J. F., additional, Maury, A., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Motte, F., additional, Pajot, F., additional, Pascale, E., additional, Peretto, N., additional, Perotto, L., additional, Pisano, G., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A., additional, Ritacco, A., additional, Rodriguez, L., additional, Romero, C., additional, Roy, A., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2017
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28. Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance

Author

Ritacco, A., primary, Ponthieu, N., additional, Catalano, A., additional, Adam, R., additional, Ade, P., additional, André, P., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Calvo, M., additional, Coiffard, G., additional, Comis, B., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Leclercq, S., additional, Macías-Pérez, J. F., additional, Mauskopf, P., additional, Maury, A., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Rebolo-Iglesias, M., additional, Revéret, V., additional, Rodriguez, L., additional, Romero, C., additional, Ruppin, F., additional, Savini, G., additional, Schuster, K., additional, Sievers, A., additional, Thum, C., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2017
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29. Mapping the kinetic Sunyaev-Zel’dovich effect toward MACS J0717.5+3745 with NIKA

Author

Adam, R., primary, Bartalucci, I., additional, Pratt, G. W., additional, Ade, P., additional, André, P., additional, Arnaud, M., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourdin, H., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Comis, B., additional, D’Addabbo, A., additional, De Petris, M., additional, Démoclès, J., additional, Désert, F.-X., additional, Doyle, S., additional, Egami, E., additional, Ferrari, C., additional, Goupy, J., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Macías-Pérez, J.-F., additional, Maurogordato, S., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Mroczkowski, T., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Rodriguez, L., additional, Romero, C., additional, Ruppin, F., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, Zemcov, M., additional, and Zylka, R., additional

Published
2017
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30. Non-parametric deprojection of NIKA SZ observations: Pressure distribution in thePlanck-discovered cluster PSZ1 G045.85+57.71

Author

Ruppin, F., primary, Adam, R., additional, Comis, B., additional, Ade, P., additional, André, P., additional, Arnaud, M., additional, Beelen, A., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, D’Addabbo, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Leclercq, S., additional, Macías-Pérez, J. F., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pisano, G., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Pratt, G. W., additional, Revéret, V., additional, Ritacco, A., additional, Rodriguez, L., additional, Romero, C., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2017
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32. High angular resolution Sunyaev-Zel’dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis

Author

Adam, R., primary, Comis, B., additional, Bartalucci, I., additional, Adane, A., additional, Ade, P., additional, André, P., additional, Arnaud, M., additional, Beelen, A., additional, Belier, B., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, D’Addabbo, A., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Hasnoun, B., additional, Hermelo, I., additional, Kramer, C., additional, Lagache, G., additional, Leclercq, S., additional, Macías-Pérez, J.-F., additional, Martino, J., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Pratt, G. W., additional, Revéret, V., additional, Ritacco, A., additional, Rodriguez, L., additional, Savini, G., additional, Schuster, K., additional, Sievers, A., additional, Triqueneaux, S., additional, Tucker, C., additional, and Zylka, R., additional

Published
2016
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34. Pressure distribution of the high-redshift cluster of galaxies CL J1226.9+3332 with NIKA

Author

Adam, R., primary, Comis, B., additional, Macías-Pérez, J.-F., additional, Adane, A., additional, Ade, P., additional, André, P., additional, Beelen, A., additional, Belier, B., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Blanquer, G., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, Cruciani, A., additional, D’Addabbo, A., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Leclercq, S., additional, Martino, J., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Rodriguez, L., additional, Savini, G., additional, Schuster, K., additional, Sievers, A., additional, Tucker, C., additional, and Zylka, R., additional

Published
2015
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35. Performance and calibration of the NIKA camera at the IRAM 30 m telescope

Author

Catalano, A., primary, Calvo, M., additional, Ponthieu, N., additional, Adam, R., additional, Adane, A., additional, Ade, P., additional, André, P., additional, Beelen, A., additional, Belier, B., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Boudou, N., additional, Bourrion, O., additional, Coiffard, G., additional, Comis, B., additional, D’Addabbo, A., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Leclercq, S., additional, Macías-Pérez, J. F., additional, Martino, J., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Revéret, V., additional, Rodriguez, L., additional, Savini, G., additional, Schuster, K., additional, Sievers, A., additional, Tucker, C., additional, and Zylka, R., additional

Published
2014
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36. First observation of the thermal Sunyaev-Zel’dovich effect with kinetic inductance detectors

Author

Adam, R., primary, Comis, B., additional, Macías-Pérez, J. F., additional, Adane, A., additional, Ade, P., additional, André, P., additional, Beelen, A., additional, Belier, B., additional, Benoît, A., additional, Bideaud, A., additional, Billot, N., additional, Boudou, N., additional, Bourrion, O., additional, Calvo, M., additional, Catalano, A., additional, Coiffard, G., additional, D’Addabbo, A., additional, Désert, F.-X., additional, Doyle, S., additional, Goupy, J., additional, Kramer, C., additional, Leclercq, S., additional, Martino, J., additional, Mauskopf, P., additional, Mayet, F., additional, Monfardini, A., additional, Pajot, F., additional, Pascale, E., additional, Perotto, L., additional, Pointecouteau, E., additional, Ponthieu, N., additional, Revéret, V., additional, Rodriguez, L., additional, Savini, G., additional, Schuster, K., additional, Sievers, A., additional, Tucker, C., additional, and Zylka, R., additional

Published
2014
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37. Improved mm-wave photometry for kinetic inductance detectors

Author

Calvo, M., primary, Roesch, M., additional, Désert, F.-X., additional, Monfardini, A., additional, Benoit, A., additional, Mauskopf, P., additional, Ade, P., additional, Boudou, N., additional, Bourrion, O., additional, Camus, P., additional, Cruciani, A., additional, Doyle, S., additional, Hoffmann, C., additional, Leclercq, S., additional, Macias-Perez, J. F., additional, Ponthieu, N., additional, Schuster, K. F., additional, Tucker, C., additional, and Vescovi, C., additional

Published
2013
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39. XLIV. Sunyaev-Zel’dovich mapping of a low-mass cluster at z ∼ 1: a multi-wavelength approach

Author

Ricci, M., Adam, R., Eckert, D., Ade, P., André, P., Andrianasolo, A., Altieri, B., Aussel, H., Beelen, A., Benoist, C., Benoît, A., Berta, S., Bideaud, A., Birkinshaw, M., Bourrion, O., Boutigny, D., Bremer, M., Calvo, M., Cappi, A., Chiappetti, L., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Faccioli, L., Ferrari, C., Fotopoulou, S., Gastaldello, F., Giles, P., Gomez, A., Goupy, J., Hahn, O., Horellou, C., Kéruzoré, F., Koulouridis, E., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J. F., Maughan, B., Maurogordato, S., Mauskopf, P., Monfardini, A., Pacaud, F., Perotto, L., Pierre, M., Pisano, G., Pompei, E., Ponthieu, N., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Sánchez Portal, M., Schuster, K., Sereno, M., Shu, S., Sievers, A., Tucker, C., and Umetsu, K.

Subjects
Astrophysics::Cosmology and Extragalactic Astrophysics
Abstract

High-mass clusters at low redshifts have been intensively studied at various wavelengths. However, while more distant objects at lower masses constitute the bulk population of future surveys, their physical state remain poorly explored to date. In this paper, we present resolved observations of the Sunyaev-Zel’dovich (SZ) effect, obtained with the NIKA2 camera, towards the cluster of galaxies XLSSC 102, a relatively low-mass system (M500 ∼ 2 × 1014 M⊙) at z = 0.97 detected from the XXL survey. We combine NIKA2 SZ data, XMM-Newton X-ray data, and Megacam optical data to explore, respectively, the spatial distribution of the gas electron pressure, the gas density, and the galaxies themselves. We find significant offsets between the X-ray peak, the SZ peak, the brightest cluster galaxy, and the peak of galaxy density. Additionally, the galaxy distribution and the gas present elongated morphologies. This is interpreted as the sign of a recent major merging event, which induced a local boost of the gas pressure towards the north of XLSSC 102 and stripped the gas out of the galaxy group. The NIKA2 data are also combined with XXL data to construct the thermodynamic profiles of XLSSC 102, obtaining relatively tight constraints up to about ∼r500, and revealing properties that are typical of disturbed systems. We also explore the impact of the cluster centre definition and the implication of local pressure substructure on the recovered profiles. Finally, we derive the global properties of XLSSC 102 and compare them to those of high-mass-and-low-redshift systems, finding no strong evidence for non-standard evolution. We also use scaling relations to obtain alternative mass estimates from our profiles. The variation between these different mass estimates reflects the difficulty to accurately measure the mass of low-mass clusters at z ∼ 1, especially with low signal-to-noise ratio data and for a disturbed system. However, it also highlights the strength of resolved SZ observations alone and in combination with survey-like X-ray data. This is promising for the study of high redshift clusters from the combination of eROSITA and high resolution SZ instruments and will complement the new generation of optical surveys from facilities such as LSST and Euclid.\ud\udKey words: techniques: high angular resolution / galaxies: clusters: individual: XLSSC 102 / galaxies: clusters: intracluster medium / X-rays: galaxies: clusters

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40. CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping

Author

M. Béthermin, A. Gkogkou, M. Van Cuyck, G. Lagache, A. Beelen, M. Aravena, A. Benoit, J. Bounmy, M. Calvo, A. Catalano, B. de Batz de Trenquelleon, C. De Breuck, A. Fasano, A. Ferrara, J. Goupy, C. Hoarau, C. Horellou, W. Hu, A. Julia, K. Knudsen, J.-C. Lambert, J. Macias-Perez, J. Marpaud, A. Monfardini, A. Pallottini, N. Ponthieu, Y. Roehlly, L. Vallini, F. Walter, A. Weiss, 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), ANR-11-IDEX-0001,Amidex,INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE(2011), European Project: PE9, ERC-2017-ADG, Intensity mapping of the atomic carbon CII line: the promise of a new observational probe of dusty star-formation in post-reionization and reionization epoch,Advanced Grant (AdG), PE9, ERC-2017-ADG,CONCERTO(2017), Bethermin, M., Gkogkou, A., Van Cuyck, M., Lagache, G., Beelen, A., Aravena, M., Benoit, A., Bounmy, J., Calvo, M., Catalano, A., De Batz De Trenquelleon, B., De Breuck, C., Fasano, A., Ferrara, A., Goupy, J., Hoarau, C., Horellou, C., Hu, W., Julia, A., Knudsen, K., Lambert, J. -C., Macias-Perez, J., Marpaud, J., Monfardini, A., Pallottini, A., Ponthieu, N., Roehlly, Y., Vallini, L., Walter, F., Weiss, A., Observatoire astronomique de Strasbourg (ObAS), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Institut Néel (NEEL), 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)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), 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 ), Cryogénie (NEEL - Cryo), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), and Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), Large-scale structure of Universe, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Cosmic background radiation, star formation [Galaxies], Astrophysics - Astrophysics of Galaxies, high-redshift [Galaxies], Settore FIS/05 - Astronomia e Astrofisica, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), ISM [Galaxies], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The intensity mapping of the [CII] 158um line redshifted to the sub-mm window is a promising probe of the z>4 star formation and its spatial distribution into the large-scale structure. To prepare the first-generation experiments (e.g., CONCERTO), we need realistic simulations of the sub-mm extragalactic sky in spectroscopy. We present a new version of the SIDES simulation including the main sub-mm lines around 1mm (CO, [CII], [CI]). This approach successfully reproduces the observed line luminosity functions. We then use our simulation to generate CONCERTO-like cubes (125-305GHz) and forecast the power spectra of the fluctuations caused by the various astrophysical components at those frequencies. Depending on our assumptions on the relation between star formation rate and [CII] luminosity, and the star formation history, our predictions of the z~6 [CII] power spectrum vary by two orders of magnitude. This highlights how uncertain the predictions are and how important future measurements will be to improve our understanding of this early epoch. SIDES can reproduce the CO shot noise recently measured at ~100 GHz by the mmIME experiment. Finally, we compare the contribution of the different astrophysical components at various redshift to the power spectra. The continuum is by far the brightest, by a factor of 3 to 100 depending on the frequency. At 300GHz, the CO foreground power spectrum is higher than the [CII] one for our base scenario. At lower frequency, the contrast between [CII] and extragalactic foregrounds is even worse. Masking the known galaxies from deep surveys should allow to reduce the foregrounds to 20% of the [CII] power spectrum up to z~6.5. However, this masking method will not be sufficient at higher redshifts. The code and the products of our simulation are released publicly and can be used for both intensity mapping experiments and sub-mm continuum and line surveys., 28 pages, 19 figures, 2 tables, accepted by A&A, the code and the products are available at https://cesamsi.lam.fr/instance/sides/home

Published
2022
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