1. CONCERTO at APEX: Installation and first phase of on-sky commissioning
- Author
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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., Duràn, 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., Macìas-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
Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - 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 post-reionisation epoch (4.5
- Published
- 2021
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