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The Detector System for the Stratospheric Kinetic Inductance Polarimeter (SKIP)

Johnson, B. R. and Ade, P. A. R. and Araujo, D. and Bradford, K. J. and Chapman, D. and Day, P. K. and Didier, J. and Doyle, S. and Eriksen, H. K. and Flanigan, D. and Groppi, C. and Hillbrand, S. and Jones, G. and Limon, M. and Mauskopf, P. and McCarrick, H. and Miller, A. and Mroczkowski, T. and Reichborn-Kjennerud, B. and Smiley, B. and Sobrin, J. and Wehus, I. K. and Zmuidzinas, J. (2014) The Detector System for the Stratospheric Kinetic Inductance Polarimeter (SKIP). Journal of Low Temperature Physics, 176 (5-6). pp. 741-748. ISSN 0022-2291. https://resolver.caltech.edu/CaltechAUTHORS:20140905-081044803

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Abstract

The stratospheric kinetic inductance polarimeter is a proposed balloon-borne experiment designed to study the cosmic microwave background, the cosmic infrared background and Galactic dust emission by observing 1,133 deg^2 of sky in the Northern Hemisphere with launches from Kiruna, Sweden. The instrument contains 2,317 single-polarization, horn-coupled, aluminum lumped-element kinetic inductance detectors (Lekids). The Lekids will be maintained at 100 mK with an adiabatic demagnetization refrigerator. The polarimeter operates in two configurations, one sensitive to a spectral band centered on 150 GHz and the other sensitive to 260 and 350 GHz bands. The detector readout system is based on the ROACH-1 board, and the detectors will be biased below 300 MHz. The detector array is fed by an F/2.4 crossed-Dragone telescope with a 500 mm aperture yielding a 15 arcmin FWHM beam at 150 GHz. To minimize detector loading and maximize sensitivity, the entire optical system will be cooled to 1 K. Linearly polarized sky signals will be modulated with a metal-mesh half-wave plate that is mounted at the telescope aperture and rotated by a superconducting magnetic bearing. The observation program consists of at least two, 5-day flights beginning with the 150 GHz observations.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/s10909-013-1014-3DOIArticle
http://rdcu.be/tvQ0PublisherFree ReadCube access
http://arxiv.org/abs/1308.0235arXivDiscussion Paper
ORCID:
AuthorORCID
Ade, P. A. R.0000-0002-5127-0401
Jones, G.0000-0002-0267-9024
Limon, M.0000-0002-5900-2698
Mroczkowski, T.0000-0003-3816-5372
Additional Information:© 2013 Springer Science+Business Media New York. Received: 31 July 2013. Accepted: 6 December 2013. Published online: 25 December 2013.
Subject Keywords:CMB, CIB, MKID, LEKID
Issue or Number:5-6
Record Number:CaltechAUTHORS:20140905-081044803
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140905-081044803
Official Citation:Johnson, B.R., Ade, P.A.R., Araujo, D. et al. J Low Temp Phys (2014) 176: 741. doi:10.1007/s10909-013-1014-3
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:49265
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:05 Sep 2014 16:52
Last Modified:13 Nov 2019 20:21

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