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  SPIDER: CMB Polarimetry from the Edge of Space

Gualtieri, R., Filippini, J. P., Ade, P. A. R., Amiri, M., Benton, S. J., Bergman, A. S., et al. (2018). SPIDER: CMB Polarimetry from the Edge of Space. Journal of Low Temperature Physics, 193, 1112-1121.

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Gualtieri, R.1, Author
Filippini, J. P.1, Author
Ade, P. A. R.1, Author
Amiri, M.1, Author
Benton, S. J.1, Author
Bergman, A. S.1, Author
Bihary, R.1, Author
Bock, J. J.1, Author
Bond, J. R.1, Author
Bryan, S. A.1, Author
Chiang, H. C.1, Author
Contaldi, C. R.1, Author
Doré, O.1, Author
Duivenvoorden, A. J.1, Author
Eriksen, H. K.1, Author
Farhang, M.1, Author
Fissel, L. M.1, Author
Fraisse, A. A.1, Author
Freese, K.1, Author
Galloway, M.1, Author
Gambrel, A. E.1, AuthorGandilo, N. N.1, AuthorGanga, K.1, AuthorGramillano, R. V.1, AuthorGudmundsson, J. E.1, AuthorHalpern, M.1, AuthorHartley, J.1, AuthorHasselfield, M.1, AuthorHilton, G.1, AuthorHolmes, W.1, AuthorHristov, V. V.1, AuthorHuang, Z.1, AuthorIrwin, K. D.1, AuthorJones, W. C.1, AuthorKuo, C. L.1, AuthorKermish, Z. D.1, AuthorLi, S.1, AuthorMason, P. V.1, AuthorMegerian, K.1, AuthorMoncelsi, L.1, AuthorMorford, T. A.1, AuthorNagy, J. M.1, AuthorNetterfield, C. B.1, AuthorNolta, M.1, AuthorOsherson, B.1, AuthorPadilla, I. L.1, AuthorRacine, B.1, AuthorRahlin, A. S.1, AuthorReintsema, C.1, AuthorRuhl, J. E.1, AuthorRunyan, M. C.1, AuthorRuud, T. M.1, AuthorShariff, J. A.1, AuthorSoler, J. D.1, AuthorSong, X.1, AuthorTrangsrud, A.1, AuthorTucker, C.1, AuthorTucker, R. S.1, AuthorTurner, A. D.1, AuthorList, J. F. van der1, AuthorWeber, A. C.1, AuthorWehus, I. K.1, AuthorWiebe, D. V.1, AuthorYoung, E. Y.1, Author more..
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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Free keywords: Cosmic microwave background Inflation Bolometers Transition-edge sensors Polarimetry Astrophysics - Cosmology and Nongalactic Astrophysics Astrophysics - Instrumentation and Methods for Astrophysics
 Abstract: Spider is a balloon-borne instrument designed to map the polarization of the millimeter-wave sky at large angular scales. Spider targets the B-mode signature of primordial gravitational waves in the cosmic microwave background (CMB), with a focus on mapping a large sky area with high fidelity at multiple frequencies. Spider 's first long- duration balloon (LDB) flight in January 2015 deployed a total of 2400 antenna-coupled transition-edge sensors (TESs) at 90 GHz and 150 GHz. In this work we review the design and in-flight performance of the Spider instrument, with a particular focus on the measured performance of the detectors and instrument in a space-like loading and radiation environment. Spider 's second flight in December 2018 will incorporate payload upgrades and new receivers to map the sky at 285 GHz, providing valuable information for cleaning polarized dust emission from CMB maps.

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 Dates: 2018
 Publication Status: Issued
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Title: Journal of Low Temperature Physics
Source Genre: Journal
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Pages: - Volume / Issue: 193 Sequence Number: - Start / End Page: 1112 - 1121 Identifier: -