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Journal of Low Temperature Physics

, Volume 167, Issue 5–6, pp 834–839 | Cite as

The Néel IRAM KID Arrays (NIKA)

  • A. MonfardiniEmail author
  • A. Benoit
  • A. Bideaud
  • N. Boudou
  • M. Calvo
  • P. Camus
  • C. Hoffmann
  • F.-X. Désert
  • S. Leclercq
  • M. Roesch
  • K. Schuster
  • P. Ade
  • S. Doyle
  • P. Mauskopf
  • E. Pascale
  • C. Tucker
  • A. Bourrion
  • J. Macias-Perez
  • C. Vescovi
  • A. Barishev
  • J. Baselmans
  • L. Ferrari
  • S. J. C. Yates
  • A. Cruciani
  • P. De Bernardis
  • S. Masi
  • C. Giordano
  • B. Marghesin
  • H. G. Leduc
  • L. Swenson
Article

Abstract

We are developing an instrument based on Kinetic Inductance Detectors (KID) known as the Néel IRAM KID Array (NIKA). Leveraging the experience gained from the first generation NIKA in 2009, an improved, dual-band (150 GHz and 240 GHz) instrument has been designed and tested at the Institut of RadioAstronomie Millimetrique (IRAM) 30-meter telescope in October 2010. The performances, in terms of sensitivity on-the-sky at 150 GHz, are already comparable to existing state-of-the-art bolometer-based instruments. NIKA represents thus the first real proof that KID are a viable technology for ground-based Astronomy. We will describe the instrument, the most recent results and the future plans for building a large resident mm-wave camera.

Keywords

Low temperature detectors Kinetic inductance mm-wave astronomy 

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Copyright information

© Springer Science+Business Media, LLC 2011

Authors and Affiliations

  • A. Monfardini
    • 1
    Email author
  • A. Benoit
    • 1
  • A. Bideaud
    • 1
  • N. Boudou
    • 1
  • M. Calvo
    • 1
  • P. Camus
    • 1
  • C. Hoffmann
    • 1
  • F.-X. Désert
    • 2
  • S. Leclercq
    • 3
  • M. Roesch
    • 3
  • K. Schuster
    • 3
  • P. Ade
    • 4
  • S. Doyle
    • 4
  • P. Mauskopf
    • 4
  • E. Pascale
    • 4
  • C. Tucker
    • 4
  • A. Bourrion
    • 5
  • J. Macias-Perez
    • 5
  • C. Vescovi
    • 5
  • A. Barishev
    • 6
  • J. Baselmans
    • 6
  • L. Ferrari
    • 6
  • S. J. C. Yates
    • 6
  • A. Cruciani
    • 7
  • P. De Bernardis
    • 7
  • S. Masi
    • 7
  • C. Giordano
    • 8
  • B. Marghesin
    • 8
  • H. G. Leduc
    • 9
  • L. Swenson
    • 9
  1. 1.Institut NéelCNRS & UJFGrenobleFrance
  2. 2.IPAGUJF & CNRS-INSUGrenoble Campus, GrenobleFrance
  3. 3.IRAMSaint Martin d’HéresFrance
  4. 4.School of Physics & AstronomyCardiff UniversityCardiffUK
  5. 5.LPSC, UJF & CNRS/IN2P3 & INPGGrenobleFrance
  6. 6.SRON3584 CA Utrecht and 9700 AV GroningenThe Netherlands
  7. 7.Dipartimento di FisicaUniversità di Roma La SapienzaRomaItaly
  8. 8.Fondazione Bruno KesslerPovo (TN)Italy
  9. 9.JPL-CaltechPasadenaUSA

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