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= NIKA2 Homagepage = = NIKA2 Homepage =
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The New Instrument of Kids Arrays (NIKA2) is the next generation continuum instrument at the IRAM 30m telescope, at Pico Veleta (Spain). The instrument is based on Kinetic Inductance Detectors (KID). The instrument will allow to measure linear polarizations at 1.15 mm. NIKA2, the second generation Neel-IRAM-KID-Array, is a dual band camera operating simultaneously at 150 and 260 GHz. The instrument is based on large arrays of superconducting Kinetic Inductance Detectors (KID) operated at temperatures of 100mK. NIKA2 is built by an international consortium, led by the Institute Neel (Grenoble France).
Successful installation took place in early October 2015. NIKA2's field of view has a 6.5arcmin diameter, with angular resolutions of 12 and 18 arcsec at 1 and 2 mm wavelengths respectively. NIKA2 is designed as a facility instrument which will remain at its present position for at least a decade. The instrument will allow to measure linear polarizations at 1.15 mm.
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Somre prelimiary characteristics of NIKA-2: Some prelimiary characteristics of NIKA-2:
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 * '''1st test run''' (29-October-2015 till 10-November-2015: Installation, cool down at the 30m, testing/debugging/developing)
  * [[Nika2Run1|Go to the 1<sup>st</sup> run Wiki page]]
 * '''1^st^ test run of NIKA2''' (29-October-2015 till 10-November-2015: Installation, cool down at the 30m, testing/debugging/developing) [= Run 13 of a NIKA instrument]
  * [[Nika2Run1|Go to the 1st run Wiki page]]
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 * '''2nd test run''' (24-November-2015 till 02-December-2015: continue tests started during run 1, in particular Beam maps and NEFD with the 13 NIKEL boards assembled the last days of run 1)
  * [[Nika2Run2|Go to the 2<sup>nd</sup> run Wiki page]]
 * '''2^nd^ test run of NIKA2''' (24-November-2015 till 02-December-2015: continue tests started during run 1, in particular Beam maps and NEFD with the 13 NIKEL boards assembled the last days of run 1) [= Run 14 of a NIKA instrument]
  * [[Nika2Run2|Go to the 2nd run Wiki page]]
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 * '''3^rd^ test run of NIKA2''' (12-January-2016 till 01-February-2016: Implementation of new NIKEL boards; the 20 data lines of NIKA2 are foreseen to be plugged simultaneously. With the 3 arrays fully read, continue and redo tests started with runs 1 & 2, in particular '''Beam maps''' and NEFD. [= Run 15 of a NIKA instrument]
  * [[Nika2Run3|Go to the 3rd run Wiki page]]


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NIKA2 Homepage

NIKA2, the second generation Neel-IRAM-KID-Array, is a dual band camera operating simultaneously at 150 and 260 GHz. The instrument is based on large arrays of superconducting Kinetic Inductance Detectors (KID) operated at temperatures of 100mK. NIKA2 is built by an international consortium, led by the Institute Neel (Grenoble France). Successful installation took place in early October 2015. NIKA2's field of view has a 6.5arcmin diameter, with angular resolutions of 12 and 18 arcsec at 1 and 2 mm wavelengths respectively. NIKA2 is designed as a facility instrument which will remain at its present position for at least a decade. The instrument will allow to measure linear polarizations at 1.15 mm.

Go to the Front Page


Overview

Some prelimiary characteristics of NIKA-2:

Band

Number of KIDs

Wavelength

Bandwidth

NEFD (goal, TBC)

HPBW

FoV

NIKA2 2 mm/150 GHz

1020

2.00 mm

125-170 GHz

TBC mJy*s1/2

TBC

6.5'

NIKA2 1 mm/260 GHz

2x1140

1.15 mm

240-280 GHz

TBC mJy*s1/2

TBC

6.5'


Technical Documentation


Technical runs

  • 1st test run of NIKA2 (29-October-2015 till 10-November-2015: Installation, cool down at the 30m, testing/debugging/developing) [= Run 13 of a NIKA instrument]

  • 2nd test run of NIKA2 (24-November-2015 till 02-December-2015: continue tests started during run 1, in particular Beam maps and NEFD with the 13 NIKEL boards assembled the last days of run 1) [= Run 14 of a NIKA instrument]

  • 3rd test run of NIKA2 (12-January-2016 till 01-February-2016: Implementation of new NIKEL boards; the 20 data lines of NIKA2 are foreseen to be plugged simultaneously. With the 3 arrays fully read, continue and redo tests started with runs 1 & 2, in particular Beam maps and NEFD. [= Run 15 of a NIKA instrument]


Publications on NIKA-1

  • Technical papers:
    • Catalano, A., Goupy, J., Le Sueur, H., et al, 2015, A&A submitted

    • Monfardini, A., Adam, R., Adane, A., et al, 2014, JLTP, Vol. 176, Issue 5-6, pp. 787-795
    • Bourrion, O., Vescovi, C., Catalano, A. et al, 2013, Journ. of Instr., Vol. 8, Issue 12, article id. C12006
    • Bourrion, O., Vescovi, C., Bouly J.-L. et al, 2012, Journ. of Instr., Vol. 7, Issue 07, pp. 7014
    • Bourrion, O., Bideaud, A., Benoit, A., et al, 2011, Journ. of Instr., Vol. 6, Issue 06, pp. 6012
  • Astronomical papers:
    • Adam, A., Comis, B., Macias-Perez, J.-F., et al, 2015, A&A, 576, A12

    • Catalano, A., Ponthieu, N., Calvo M., et al, 2014, A&A, 569, A9

    • Adam, R., Comis, B., Macias-Perez, J.-F, et al, 2014, A&A in press

    • Calvo, M., Roesh, M., Désert, F.-X., et al, 2013, A&A, 551, L12

    • Monfardini, A., Benoit, A., Bideaud, A., et al, 2011, ApJs, 194, 24

    • Monfardini, A., Swenson, L. J., Bideaud, A., et al, 2010, AAp, 521, A29


Support teams


Author: Israel Hermelo (IRAM 30m continuum pool manager)

email: hermelo@iram.es

Created: 2015.AUG.05

This page is maintained by IH, CK, SL and the NIKA team

Last update: 2015.OCT.19

Continuum/NIKA2/Main (last edited 2025-02-21 12:02:51 by CarstenKramer)