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=== Commissioning (October 2015) ===

[[http://www.iram.es/IRAMES/mainWiki/Continuum/NIKA2/Commissioning | Go to the NIKA2 commissioning wiki]]

=== Installation (September 2015) ===

[[http://www.iram.es/IRAMES/mainWiki/Continuum/NIKA2/Installation | Go to the NIKA2 installation wiki]]
 * '''1st test run''' (October 2015, Installation, 1st cool down at the 30m, start commissioning procedures)
  * [[Nika2Run1|Go to the 1st run Wiki page]]
  * [[http://www.iram.fr/wiki/nika2/index.php/CommissioningNIKA2 | Private Wiki detailing the organization of the run and the commissioning plan]]
  * (IH started a [[http://www.iram.es/IRAMES/mainWiki/Continuum/NIKA2/Commissioning | public commissioning wiki page, now obsolete]] to be removed ?)
  * (IH started a [[http://www.iram.es/IRAMES/mainWiki/Continuum/NIKA2/Installation | public installation wiki page, now obsolete]] to be removed ?)

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 (KIDS). The baseline detector focal plane units consist of 1000 detectors at 2 mm and 4000 detectors at 1.25 mm. The instrument will provide the measurement of the linear polarization at 1.25 mm.

Go to the Front Page


Overview

The main characteristics of the latest configuration (2015.AUG.05) are summarized on the following table.

Band

Number of KIDs

Wavelength

Bandwidth

NEFD

HPBW

FoV

NIKA 2 mm

1000

2.0 mm

xxx GHz

10 mJy*s1/2

18.5"

6.5'

NIKA 1 mm

2x2000

1.2 mm

xxx GHz

15 mJy*s1/2

11.0"

6.5'


Call for proposals

NIKA2 is not offered to the community yet.


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 the continuum cameras as well as examples of the scripts that you need to prepare to observe your project.

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

  • Pointing sources and calibrators provides a list of pointing sources and calibrators for the IRAM 30m continuum cameras.

  • Observe GRBs


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.AUG.05

Continuum/NIKA2/Main (last edited 2025-04-02 15:43:17 by NikaBolometer)