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<z<8.5), and on studying galaxy clusters via the thermal and kinetic Sunyaev-Zel’dovich (SZ) effect. CONCERTO will also measure the dust and molecular gas contents of local and intermediate-redshift galaxies, it will study the Galactic star-forming clouds and finally it will observe the CO intensity fluctuations arising from 0.3<z<2 galaxies.

The design of the instrument, installation at APEX and current status of the commissioning phase and science verification will be presented. Also we describe the deployment and first on-sky tests performed between April and June 2021.

Details

Title
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; F.-X. Désert; Durán, C A; Duvauchelle, G; Eraud, L; Fasano, A; Fenouillet, T; Garcia, J; Garde, G; Goupy, J; Groppi, C; Hoarau, C; W. Hu; Lagache, G; J.-C. Lambert; J.-P. Leggeri; 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; Vivargent, L
Publication year
2022
Publication date
2022
Publisher
EDP Sciences
ISSN
21016275
e-ISSN
2100014X
Source type
Conference Paper
Language of publication
English
ProQuest document ID
3191206783
Copyright
© 2022. This work is licensed under https://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the terms of the License.