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The main characteristics of the instrument installed the 29th September at Pico Veleta are: Somre prelimiary characteristics of NIKA-2:
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|| NIKA2 2 mm/150 GHz || 1020 || 2.00 mm || 125-170 GHz || 10 mJy*s^1/2^ || 18.5" || 6.5' ||
|| NIKA2 1 mm/260 GHz || 2x1140 || 1.15 mm || 240-280 GHz || 15 mJy*s^1/2^ || 12.0" || 6.5' ||
|| NIKA2 2 mm/150 GHz || 1020 || 2.00 mm || 125-170 GHz || TBC mJy*s^1/2^ || TBC || 6.5' ||
|| NIKA2 1 mm/260 GHz || 2x1140 || 1.15 mm || 240-280 GHz || TBC mJy*s^1/2^ || TBC || 6.5' ||
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 * [[http://ipag.osug.fr/nika2/Welcome.html | NIKA2 official website ]]
 * [[http://www.iram.fr/wiki/nika2/index.php/Nika2Wiki | Private wiki]].
 * Web information in France:
  
* [[http://ipag.osug.fr/nika2/Welcome.html | NIKA2 website at IPAG ]]
   * [[http://www.iram.fr/wiki/nika2/index.php/Nika2Wiki | IRAM-internal wiki at IRAM-FR ]].
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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 2nd run Wiki page]]

NIKA2 Homagepage

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.

Go to the Front Page


Overview

Somre 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

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)