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26 April 2024
 
  » arxiv » 1004.2209

 Article overview



NIKA: A Millimeter-Wave Kinetic Inductance Camera
A. Monfardini ; L. J. Swenson ; A. Bideaud ; F. X. Désert ; S. J. C. Yates ; A. Benoit ; A. M. Baryshev ; J. J. A. Baselmans ; S. Doyle ; B. Klein ; M. Roesch ; C. Tucker ; P. Ade ; M. Calvo ; P. Camus ; C. Giordano ; R. Guesten ; C. Hoffmann ; S. Leclercq ; P. Mauskopf ; K. F. Schuster ;
Date 13 Apr 2010
AbstractCurrent generation millimeter wavelength detectors suffer from scaling limits imposed by complex cryogenic readout electronics. To circumvent this it is imperative to investigate technologies that intrinsically incorporate strong multiplexing. One possible solution is the Kinetic-Inductance Detector (KID). In order to assess the potential of this nascent technology, a prototype instrument optimized for the 2 mm atmospheric window was constructed. Known as the N’eel IRAM KIDs Array (NIKA), it was recently tested at the Institute for Millimetric Radio Astronomy (IRAM) 30-meter telescope at Pico Veleta, Spain. The measurement resulted in the imaging of a number of sources, including planets, quasars, and galaxies. The images for Mars, radio star MWC349, quasar 3C345, and galaxy M87 are presented. From these results, the optical NEP was calculated to be around $1 imes 10^{-15}$ W$ / $Hz$^{1/2}$. A factor of 10 improvement is expected to be readily feasible by improvements in the detector materials and reduction of performance-degrading spurious radiation.
Source arXiv, 1004.2209
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