The NIKA 2013-2014 observation campaigns: control of systematic effects and results

Catalano, A., Adam, R., Adane, A., Ade, P. ORCID: https://orcid.org/0000-0002-5127-0401, Andre, P., Beelen, A., Belier, B., Benoit, A., Bideaud, A., Billot, N., Boudou, N., Bourrion, O., Calvo, M., Coiffard, G., Comis, B., D'Addabbo, A., Desert, F. -X., Doyle, S., Kramer, C., Leclercq, S., Macias-Perez, J. -F., Martino, J., Mauskopf, P. ORCID: https://orcid.org/0000-0001-6397-5516, Mayet, F., Monfardini, A., Pajot, F., Pascale, E., Perotto, L., Pointecouteau, E., Ponthieu, N., Reveret, V., Ritacco, A., Rodriguez, L., Savini, G., Schuster, K., Sievers, A., Tucker, C. ORCID: https://orcid.org/0000-0002-1851-3918 and Zylka, R. 2014. The NIKA 2013-2014 observation campaigns: control of systematic effects and results. Presented at: SPIE Astronomical Telescopes + Instrumentation 2014, Montreal, Canada, 22-27 June 2014. Proceedings Volume 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. , vol.9153 SPIE, p. 915302. 10.1117/12.2055403

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Abstract

The New IRAM KID Array (NIKA) is a dual-band camera operating with frequency multiplexed arrays of Lumped Element Kinetic Inductance Detectors (LEKIDs) cooled to 100 mK. NIKA is designed to observe the intensity and polarisation of the sky at 1.25 and 2.14 mm from the IRAM 30 m telescope. We present the improvements on the control of systematic effects and astrophysical results made during the last observation campaigns between 2012 and 2014.

Item Type:	Conference or Workshop Item (UNSPECIFIED)
Status:	Published
Schools:	Schools > Physics and Astronomy
Publisher:	SPIE
Last Modified:	24 Oct 2025 21:54
URI:	https://orca.cardiff.ac.uk/id/eprint/156654

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