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||NIKA 1mm band || 132 (125 valid) || 2.00 mm || 137-172 GHz || 14 mJy*s^1/2^ (preliminary) || 17.5" || 1.9' || 9.8" ||
||NIKA 2mm band || 224 (190 valid) || 1.25 mm || 220-270 GHz || 35 mJy*s^1/2^ (preliminary) || 12.0" || 1.8' || 6.8" ||
||NIKA 2mm band || 132 (125 valid) || 2.00 mm || 137-172 GHz || 14 mJy*s^1/2^ (preliminary) || 17.5" || 1.9' || 9.8" ||
||NIKA 1mm band || 224 (190 valid) || 1.25 mm || 220-270 GHz || 35 mJy*s^1/2^ (preliminary) || 12.0" || 1.8' || 6.8" ||

NIKA

The New IRAM KIDs Array (NIKA) is a Kinetic Inductance Detectors camera for bolometric observations at the IRAM 30m telescope. NIKA has been built by the Institut Néel (IN) and LPSC in Grenoble, France under the lead of Alain Benoit, and with the contributions of other persons forming the NIKA collaboration. In 2013 the main contributing institutes are IN, IRAM, IPAG, LPSC, AIG Cardiff.

Go to the Front Page


Overview

NIKA is a dual band instrument using few hundreds of Kinetic Inductance Detectors (KID). The KID resonances variations which are dependent on the incoming power are probed by a comb of tones allowing to perform frequency domain multiplexing. Being a prototype in constant evolution the arrays characteristics (number of pixels, field of view, sensitivity, etc.) have evolved over the years from each test run to the other. The main characteristics of the latest configuration are summarized on the following table.

Parameters from run 6

Number of KIDs

Wavelength

Bandwidth (FWHM)

Sensitivity (out of atmosphere)

HPBW

Field-of-View diameter

Spacing

NIKA 2mm band

132 (125 valid)

2.00 mm

137-172 GHz

14 mJy*s1/2 (preliminary)

17.5"

1.9'

9.8"

NIKA 1mm band

224 (190 valid)

1.25 mm

220-270 GHz

35 mJy*s1/2 (preliminary)

12.0"

1.8'

6.8"

NIKA is a prototype used to test the technologies to be used in the bigger 6.5' FOV NIKA2 instrument currently in development phase (private Wiki here).

For IRAM personnel: Procedure for cooling down the PT NIKA cryostat.


Call for proposals

NIKA is offered for the first time to the community the winter semester 2013/14:


Publications


Support teams


NIKA 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.

  • Calibrators (coming soon) provides flux measurements of primary and secondary calibrators for the IRAM 30m continuum cameras.

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

  • Alignment and pointing sesion (in prep.) provides a step-by-step method to establish a good pointing with NIKA.

  • Data Reduction (coming soon) provides some basic examples to reduce NIKA data.


1st NIKA pool (February 2014)

The 1st NIKA pool will take place from the 18th of February to the 28th of February 2014.

Pool projects and observers

For information about the accepted projects and the observers at the 30m please go to:

Progress

The progress of the pool can be followed via:

Both databases are synchronized and can be used to write/read the logsheet.


Previous test and commissioning runs


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

email: hermelo@iram.es

Created: 2013.12.16

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

Last update: 2014.02.03

NIKA/Main (last edited 2017-02-24 18:57:16 by NikaBolometer)