Share Email Print

Proceedings Paper

Characterization of the Atacama B-mode Search
Author(s): S. M. Simon; S. Raghunathan; J. W. Appel; D. T. Becker; L. E. Campusano; H. M. Cho; T. Essinger-Hileman; S. P. Ho; K. D. Irwin; N. Jarosik; A. Kusaka; M. D. Niemack; G. W. Nixon; M. R. Nolta; L. A. Page; G. A. Palma; L. P. Parker; J. L. Sievers; S. T. Staggs; K. Visnjic
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

The Atacama B-mode Search (ABS), which began observations in February of 2012, is a crossed-Dragone telescope located at an elevation of 5190 m in the Atacama Desert in Chile. ABS is searching for the B-mode polarization spectrum of the cosmic microwave background (CMB) at large angular scales from multipole moments of ` ~ 50 ~ 500, a range that includes the primor- dial B-mode peak from inflationary gravity waves at ~ 100. The ABS focal plane consists of 240 pixels sensitive to 145 GHz, each containing two transition-edge sensor bolometers coupled to orthogonal polarizations with a planar ortho-mode transducer. An ambient-temperature con- tinuously rotating half-wave plate and 4 K optics make the ABS instrument unique. We discuss the characterization of the detector spectral responses with a Fourier transform spectrometer and demonstrate that the pointing model is adequate. We also present measurements of the beam from point sources and compare them with simulations.

Paper Details

Date Published: 23 July 2014
PDF: 15 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 91530Y (23 July 2014); doi: 10.1117/12.2055576
Show Author Affiliations
S. M. Simon, Princeton Univ. (United States)
S. Raghunathan, Univ. de Chile (Chile)
J. W. Appel, Johns Hopkins Univ. (United States)
D. T. Becker, National Institute of Standards and Technology (United States)
L. E. Campusano, Univ. de Chile (Chile)
H. M. Cho, National Institute of Standards and Technology (United States)
T. Essinger-Hileman, Johns Hopkins Univ. (United States)
S. P. Ho, Princeton Univ. (United States)
K. D. Irwin, National Institute of Standards and Technology (United States)
Stanford Univ. (United States)
N. Jarosik, Princeton Univ. (United States)
A. Kusaka, Princeton Univ. (United States)
M. D. Niemack, Cornell Univ. (United States)
G. W. Nixon, Princeton Univ. (United States)
M. R. Nolta, The Canadian Institute for Theoretical Astrophysics, Univ. of Toronto (Canada)
L. A. Page, Princeton Univ. (United States)
G. A. Palma, Univ. de Chile (Chile)
L. P. Parker, Princeton Univ. (United States)
J. L. Sievers, Univ. of KwaZulu-Natal (South Africa)
S. T. Staggs, Princeton Univ. (United States)
K. Visnjic, Princeton Univ. (United States)

Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?