4.2 Article

Latest NIKA Results and the NIKA-2 Project

Journal

JOURNAL OF LOW TEMPERATURE PHYSICS
Volume 176, Issue 5-6, Pages 787-795

Publisher

SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10909-013-0985-4

Keywords

Kinetic inductance detectors; Millimeter astronomy; Superconducting detectors

Funding

  1. Foundation Nanoscience Grenoble
  2. ANR under MKIDS
  3. ANR under NIKA
  4. LabEx FOCUS [ANR-11-LABX-0013]
  5. European Research Council Advanced Grant ORISTARS under the European Union [291294]
  6. STFC [ST/K000926/1] Funding Source: UKRI
  7. Science and Technology Facilities Council [ST/K000926/1] Funding Source: researchfish

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NIKA (New IRAM KID Arrays) is a dual-band imaging instrument installed at the IRAM (Institut de RadioAstronomie Millimetrique) 30-meter telescope at Pico Veleta (Spain). Two distinct Kinetic Inductance Detectors (KID) focal planes allow the camera to simultaneous image a field-of-view of about 2 arc-min in the bands 125 to 175 GHz (150 GHz) and 200 to 280 GHz (240 GHz). The sensitivity and stability achieved during the last commissioning Run in June 2013 allows opening the instrument to general observers. We report here the latest results, in particular in terms of sensitivity, now comparable to the state-of-the-art Transition Edge Sensors (TES) bolometers, relative and absolute photometry. We describe briefly the next generation NIKA-2 instrument, selected by IRAM to occupy, from 2015, the continuum imager/polarimeter slot at the 30-m telescope.

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