Differences between revisions 25 and 29 (spanning 4 versions)
Revision 25 as of 2015-11-11 11:39:50
Size: 5498
Comment:
Revision 29 as of 2015-11-11 11:52:11
Size: 5648
Comment:
Deletions are marked like this. Additions are marked like this.
Line 3: Line 3:
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. 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.
Line 23: Line 23:
----

== Call for proposals ==

NIKA2 is not offered to the community yet.
## == Call for proposals ==
## NIKA2 is not offered to the community yet.
##
Line 36: Line 33:
== How-to's == == Technical Documentation ==

 * [[attachment:calvo-27oct2015-nika2-camadia.pdf | Camadia - Data Acquisition ]]

 * [[http://www.iram.es/IRAMES/mainWiki/OffProcNika2Run1Beam | Discussion on beams ]]

 * [[http://www.iram.es/IRAMES/mainWiki/Spectral%20bands | Spectral bands ]]

 * [[http://www.iram.es/IRAMES/mainWiki/Continuum/NetworkAccess | Remote network access to NIKA-2 ]]
Line 43: Line 48:

 * [[http://www.iram.es/IRAMES/mainWiki/Continuum/NetworkAccess | Remote network access to NIKA-2 ]]
Line 69: Line 72:
 * '''1st test run''' (October 2015, Installation, 1st cool down at the 30m, start commissioning procedures)  * '''1st test run''' (29-October-2015 till 10-November-2015: Installation, cool down at the 30m, testing/debugging/developing)

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

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'


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)