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The New IRAM KIDs Array (NIKA) is a Kinetic Inductance Detectors camera for bolometric observations at the IRAM 30m telescope. This 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 above table.
 NIKA has been built by the Institut Néel (IN), 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.
The New IRAM KIDs Array (NIKA) is a Kinetic Inductance Detectors camera for bolometric observations at the IRAM 30m telescope. This 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 above table. <<BR>>
NIKA has been built by the Institut Néel (IN), 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.

NIKA

This page is maintained by CK and SL


NIKA-1 Overview

Pixels

Wavelength

Bandwidth

Sensitivity

HPBW

Field-of-View

Spacing

NIKA-1 run 6

132 (128 valid)

2 mm

122-166 GHz

15 mJy*s1/2 (preliminary)

18.5"

2.3' diameter

9.8"

NIKA-1 run 6

224 (190 valid)

1.25 mm

213-251 GHz

51 mJy*s1/2 (preliminary

12.5"

2.3' diameter

6.8"

The New IRAM KIDs Array (NIKA) is a Kinetic Inductance Detectors camera for bolometric observations at the IRAM 30m telescope. This 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 above table.
NIKA has been built by the Institut Néel (IN), 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.

Publications

Team

Test runs 2009-2013

6th test run, June 2013

Go to the 6th run Wiki page

5th test run, November 2012

Go to the 5th run Wiki page

4th test run, June 2012

Go to the 4th run Wiki page

3rd test run, October 2011

Go to the 3rd run Wiki page

2nd test run, October 2010

Go to the 2nd run Wiki page

1st test run, October 2009

Go to the 1st run Wiki page

Procedure for cooling down the PT NIKA cryostat

See page dedicated to this procedure


NIKA-2

NIKA-1 is a 2.3' FOV prototype used to test the technologies to be used in the bigger 6.5' FOV NIKA-2 instrument currently in development phase.

NIKA-2 development dedicated private Wiki