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Last update: 2015.OCT.05 Last update: 2015.OCT.19

NIKA2

The New Instrument of Kids Arrays (NIKA2) is the next generation continuum instrument to be placed at the 30m telescope of IRAM, at Pico Veleta (Spain). The instrument is based on Kinetic Inductance Detectors (KID). The baseline detector focal plane units consist of 1020 detectors at 2 mm and 2x1140 detectors at 1.15 mm. The instrument will provide the measurement of the linear polarization at 1.15 mm.

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Overview

The main characteristics of the instrument installed the 29th September at Pico Veleta are:

Band

Number of KIDs

Wavelength

Bandwidth

NEFD (goal, TBC)

HPBW

FoV

NIKA2 2 mm/150 GHz

1020

2.00 mm

125-170 GHz

10 mJy*s1/2

18.5"

6.5'

NIKA2 1 mm/260 GHz

2x1140

1.15 mm

240-280 GHz

15 mJy*s1/2

12.0"

6.5'


Call for proposals

NIKA2 is not offered to the community yet. It is being commissioned during Oct 2015 until mid 2016.


Publications

  • 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


How-to's

  • Pool Preparation provides information on the observing modes offered for NIKA2 and examples of the scripts that you must prepare to observe your project.

  • Observing Session provides an example of a typical session with NIKA2 at the 30m telescope.

  • Pointing sources and calibrators provides a list of pointing sources and calibrators.


Technical runs


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)