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1. CONCERTO at APEX: Installation and Technical Commissioning

Author

Monfardini, A., Beelen, A., Benoit, A., Bounmy, J., Calvo, M., Catalano, A., Goupy, J., Lagache, G., Ade, P., Barria, E., Béthermin, M., Bourrion, O., Bres, G., Breuck, C. De, Désert, F. -X., Duvauchelle, G., Fasano, A., Fenouillet, T., Garcia, J., Garde, G., Hoarau, C., Hu, W., Lambert, J. -C., Levy-Bertrand, F., Lundgren, A., Macias-Perez, J., Marpaud, J., Pisano, G., Ponthieu, N., Prieur, L., Roni, S., Roudier, S., Tourres, D., Tucker, C., Cantzler, M., Caro, P., Diaz, M., Durán, C., Montenegro, F., Navarro, M., Olguin, R., Palma, F., Parra, R., and Santana, J.

Published
2022
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2. The KISS Experiment

Author

Fasano, A., Aguiar, M., Benoit, A., Bideaud, A., Bourrion, O., Calvo, M., Catalano, A., de Taoro, A. P., Garde, G., Gomez, A., Gomez Renasco, M. F., Goupy, J., Hoarau, C., Hoyland, R., Macías-Pérez, J. F., Marpaud, J., Monfardini, A., Pisano, G., Ponthieu, N., Rubiño Martín, J. A., Tourres, D., Tucker, C., Beelen, A., Bres, G., De Petris, M., de Bernardis, P., Lagache, G., Lamagna, L., Luzzi, G., Marton, M., Masi, S., Rebolo, R., and Roudier, S.

Published
2020
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4. CONCERTO at APEX: Installation and first phase of on-sky commissioning

Author

Catalano A., Ade P., Aravena M., Barria E., Beelen A., Benoit A., Béthermin M., Bounmy J., Bourrion O., Bres G., De Breuck C., Calvo M., Désert F.-X., Durán C.A, Duvauchelle G., Eraud L., Fasano A., Fenouillet T., Garcia J., Garde G., Goupy J., Groppi C., Hoarau C., Hu W., Lagache G., Lambert J.-C., Leggeri J.-P., Levy-Bertrand F., Macías-Pérez J., Mani H., Marpaud J., Marton M., Mauskopf P., Monfardini A., Pisano G., Ponthieu N., Prieur L., Raffin G., Roni S., Roudier S., Tourres D., Tucker C., and Vivargent L.

Subjects
Physics, QC1-999
Abstract

CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn) is a large field-of-view (FoV) spectro-imager that has been installed on the Cassegrain Cabin of Atacama Pathfinder EXperiment (APEX) telescope in April 2021. CONCERTO hosts 2 focal planes and a total number of 4000 Kinetic Inductance Detectors (KID), with an instantaneous FoV of 18.6 arcminutes in the range of 130-310 GHz. The spectral resolution can be easily tuned down to 1 GHz depending on the scientific target. The scientific program of CONCERTO has many objectives, with two main programs focused on mapping the fluctuations of the [CII] line intensity in the reionisation and postreionisation epoch (4.5

Published
2022
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5. Observations with KIDs Interferometer Spectrum Survey (KISS)

Author

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

Subjects
Physics, QC1-999
Abstract

We describe the preliminary on-sky results of the KIDs Interferometer Spectrum Survey (KISS), a spectral imager with a 1 deg field of view (FoV). The instrument operates in the range 120–180 GHz from the 2.25m Q-U-I JOint TEnerife telescope in Teide Observatory (Tenerife, Canary Islands), at 2 395m altitude above sea level. Spectra at low resolution, up to 1.45 GHz, are obtained using a fast (3.72 Hz mechanical frequency) Fourier transform spectrometer, coupled to a continuous dilution cryostat with a stabilized temperature of 170mK that hosts two 316-pixel arrays of lumped-element kinetic inductance detectors. KISS generates more than 3 000 spectra per second during observations and represents a pathfinder to demonstrate the potential for spectral mapping with large FoV.We give an overall description of the spectral mapping paradigm and we present recent results from observations, in this paper.

Published
2022
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6. The NIKA2 Instrument at 30-m IRAM Telescope: Performance and Results

Author

Catalano, A., Adam, R., Ade, P. A. R., André, P., Aussel, H., Beelen, A., Benoît, A., Bideaud, A., Billot, N., Bourrion, O., Calvo, M., Comis, B., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Goupy, J., Kramer, C., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J. F., Mauskopf, P., Mayet, F., Monfardini, A., Pascale, E., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Triqueneaux, S., Tucker, C., Zylka, R., Barria, E., Bres, G., Camus, P., Chanthib, P., Donnier-Valentin, G., Exshaw, O., Garde, G., Gerardin, A., Leggeri, J.-P., Levy-Bertrand, F., Guttin, C., Hoarau, C., Grollier, M., Mocellin, J.-L., Pont, G., Rodenas, H., Tissot, O., Galvez, G., John, D., Ungerechts, H., Sanchez, S., Mellado, P., Munoz, M., Pierfederici, F., Penalver, J., Navarro, S., Bosson, G., Bouly, J.-L., Bouvier, J., Geraci, C., Li, C., Menu, J., Ponchant, N., Roni, S., Roudier, S., Scordillis, J. P., Tourres, D., Vescovi, C., Barbier, A., Billon-Pierron, D., Adane, A., Andrianasolo, A., Bracco, A., Coiffard, G., Evans, R., Maury, A., and Rigby, A.

Published
2018
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7. The NIKA2 Instrument, A Dual-Band Kilopixel KID Array for Millimetric Astronomy

Author

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

Published
2016
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8. KISS: a spectrometric imager for millimetre cosmology

Author

Fasano A., Aguiar M., Benoit A., Bideaud A., Bourrion O., Calvo M., Catalano A., de Taoro A.P., Garde G., Gomez A., Gomez Renasco M.F., Goupy J., Hoarau C., Hoyland R., Macías-Pérez J.F., Marpaud J., Monfardini A., Pisano G., Ponthieu N., Rubiño Martín J.A., Tourres D., Tucker C., Beelen A., Bres G., De Petris M., de Bernardis P., Lagache G., Marton M., Rebolo R., and Roudier S.

Subjects
Physics, QC1-999
Abstract

Clusters of galaxies are used to map the large-scale structures in the universe and as probe of universe evolution. They can be observed through the Sunyaev-Zel’dovich (SZ) effect. In this respect the spectro-imaging at low resolution frequency is an important tool, today, for the study of cluster of galaxies. We have developed KISS (KIDs Interferometer Spectrum Survey), a spectrometric imager dedicated to the secondary anisotropies of the Cosmic Microwave Background (CMB). The multi-frequency approach permits to improve the component separation with respect to predecessor experiments. In this paper, firstly, we provide a description of the scientific context and the state of the art of SZ observations. Secondly, we describe the KISS instrument. Finally, we show preliminary results of the ongoing commissioning campaign.

Published
2020
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9. 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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