English

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

Instrumentation and Methods for Astrophysics 2015-06-22 v1

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.

Keywords

Cite

@article{arxiv.1409.0640,
  title  = {The NIKA 2012-2014 observing campaigns: control of systematic effects and results},
  author = {A. Catalano and R. Adam and A. Adane and P. Ade and P. André and A. Beelen and B. Belier and A. Benôit and A. Bideaud and N. Billot and N. Boudou and O. Bourrion and M. Calvo and G. Coiffard and B. Comis and A. D'Addabbo and F. -X. Désert and S. Doyle and J. Goupy and C. Kramer and S. Leclercq and J. F. Macías-Pérez and J. Martino and P. Mauskopf and F. Mayet and A. Monfardini and F. Pajot and E. Pascale and L. Perotto and E. Pointecouteau N. Ponthieu and V. Revéret and A. Ritacco and L. Rodriguez and G. Savini and K. Schuster and A. Sievers and C. Tucker and R. Zylka},
  journal= {arXiv preprint arXiv:1409.0640},
  year   = {2015}
}

Comments

11 pages, 17 figures, SPIE conference proceeding