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The NIKA 2012-2014 observing campaigns: control of systematic effects and results

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arxiv 1409.0640 v1 pith:XQUIZI2V submitted 2014-09-02 astro-ph.IM

The NIKA 2012-2014 observing campaigns: control of systematic effects and results

A. Catalano , R. Adam , A. Adane , P. Ade , P. Andr\'e , A. Beelen , B. Belier , A. Ben\^oit
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A. Bideaud N. Billot N. Boudou O. Bourrion M. Calvo G. Coiffard B. Comis A. D'Addabbo F.-X. D\'esert S. Doyle J. Goupy C. Kramer S. Leclercq J.F. Mac\'ias-P\'erez J. Martino P. Mauskopf F. Mayet A. Monfardini F. Pajot E. Pascale L. Perotto E. Pointecouteau N. Ponthieu V. Rev\'eret A. Ritacco L. Rodriguez G. Savini K. Schuster A. Sievers C. Tucker R. Zylka
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keywords nikacampaignscontroleffectsiramresultssystematicarray
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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.

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