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Title: The POLARBEAR Fourier transform spectrometer calibrator and spectroscopic characterization of the POLARBEAR instrument

Journal Article · · Review of Scientific Instruments
DOI:https://doi.org/10.1063/1.5095160· OSTI ID:1632130
ORCiD logo [1];  [2]; ORCiD logo [3];  [4]; ORCiD logo [2];  [5];  [6]; ORCiD logo [7];  [8];  [2]; ORCiD logo [9];  [7];  [10];  [1];  [1]; ORCiD logo [2];  [11];  [2]; ORCiD logo [10];  [2] more »;  [12];  [7]; ORCiD logo [2];  [13];  [14];  [15];  [2]; ORCiD logo [16] « less
  1. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study,The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
  2. Department of Physics, University of California, San Diego, California 92093-0424, USA
  3. Physics Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  4. Department of Physics and Astronomy, Johns Hopkins University, Baltimore, Maryland 21218, USA;Departamento de Física, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile
  5. Department of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico 87131, USA
  6. School of Physics, University of Melbourne, Parkville, VIC 3010, Australia
  7. Department of Physics, University of California, Berkeley, California 94720, USA
  8. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study,The University of Tokyo, Kashiwa, Chiba 277-8583, Japan;Department of Physics, University of California, Berkeley, California 94720, USA
  9. Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, United Kingdom
  10. High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
  11. Physics Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA;Department of Physics, University of California, Berkeley, California 94720, USA
  12. Department of Physics, Stanford University, Stanford, California 94305, USA
  13. Department of Physics, University of California, San Diego, California 92093-0424, USA;National Astronomical Research Institute of Thailand, Chiangmai, Thailand
  14. Department of Physics, Kyoto University, Kyoto 606-8502, Japan
  15. High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan;SOKENDAI (The Graduate University for Advanced Studies), Shonan Village, Hayama, Kanagawa 240-0193, Japan
  16. Radio Astronomy Laboratory, University of California, Berkeley, California 94720, USA

Here we describe the Fourier Transform Spectrometer (FTS) used for in-field testing of the POLARBEAR receiver, an experiment located in the Atacama Desert of Chile which measures the cosmic microwave background (CMB) polarization. The POLARBEAR-FTS (PB-FTS) is a Martin-Puplett interferometer designed to couple to the Huan Tran Telescope (HTT) on which the POLARBEAR receiver is installed. The PB-FTS measured the spectral response of the POLARBEAR receiver with signal-to-noise ratio >20 for ~69% of the focal plane detectors due to three features: a high throughput of 15.1 sr cm2, optimized optical coupling to the POLARBEAR optics using a custom designed output parabolic mirror, and a continuously modulated output polarizer. The PB-FTS parabolic mirror is designed to mimic the shape of the 2.5 m-diameter HTT primary reflector, which allows for optimum optical coupling to the POLARBEAR receiver, reducing aberrations and systematics. One polarizing grid is placed at the output of the PB-FTS and modulated via continuous rotation. This modulation allows for decomposition of the signal into different harmonics that can be used to probe potentially pernicious sources of systematic error in a polarization-sensitive instrument. The high throughput and continuous output polarizer modulation features are unique compared to other FTS calibrators used in the CMB field. In-field characterization of the POLARBEAR receiver was accomplished using the PB-FTS in April 2014. We discuss the design, construction, and operation of the PB-FTS and present the spectral characterization of the POLARBEAR receiver. We introduce future applications for the PB-FTS in the next-generation CMB experiment, the Simons Array.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC); Japan Society for the Promotion of Science (JSPS); Comisión Nacional de Investigación Científica y Tecnológica (CONICYT); Australian Research Council; World Premier International Research Center Initiative (WPI); Ministry of Education, Culture, Sports, Science and Technology (MEXT); European Research Council (ERC)
Contributing Organization:
POLARBEAR Collaboration
Grant/Contract Number:
AC02-05CH11231; JP17F17025; 77047; 1130777; 1171811; FT150100074; 18K13558; 18H04347; 616170
OSTI ID:
1632130
Journal Information:
Review of Scientific Instruments, Vol. 90, Issue 11; ISSN 0034-6748
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 8 works
Citation information provided by
Web of Science

References (24)

Offset Multireflector Antennas with Perfect Pattern Symmetry and Polarization Discrimination journal September 1978
Joint Analysis of BICEP2/ Keck Array and Planck Data journal March 2015
The POLARBEAR experiment conference September 2012
The POLARBEAR Cosmic Microwave Background Polarization Experiment journal January 2014
The bolometric focal plane array of the POLARBEAR CMB experiment conference September 2012
A Measurement of the Cosmic Microwave Background B -mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data journal October 2017
Design and Deployment of a Multichroic Polarimeter Array on the Atacama Cosmology Telescope journal March 2016
Polarised interferometric spectrometry for the millimetre and submillimetre spectrum journal June 1970
2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization
  • Ade, Peter A.; Ahmed, Zeeshan; Aikin, Randol
  • Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX https://doi.org/10.1117/12.2313854
conference July 2018
Antenna tolerance theory—A review journal January 1966
The Quest for B Modes from Inflationary Gravitational Waves journal September 2016
Common-mode rejection in Martin–Puplett spectrometers for astronomical observations at millimeter wavelengths journal January 2015
Design for the COBE far-infrared absolute spectrophotometer
  • Mather, John C.; Fixsen, Dale J.; Shafer, Richard A.
  • SPIE's 1993 International Symposium on Optics, Imaging, and Instrumentation, SPIE Proceedings https://doi.org/10.1117/12.157823
conference October 1993
Keck array and BICEP3: spectral characterization of 5000+ detectors conference August 2014
Optical Characterization of the SPT-3G Camera journal May 2018
Transmission and reflection characteristics of slightly irregular wire-grids with finite conductivity for arbitrary angles of incidence and grid rotation journal January 2005
The Primordial Inflation Explorer (PIXIE) conference August 2014
A Survey of the Theory of Wire Grids journal May 1962
Theory of a Double Polarization Modulated Martin-Puplett Interferometer journal September 1990
The POLARBEAR-2 and Simons Array Focal Plane Fabrication Status journal September 2018
The bolometric focal plane array of the Polarbear CMB experiment text January 2012
A Joint Analysis of BICEP2/Keck Array and Planck Data text January 2015
The Quest for B Modes from Inflationary Gravitational Waves text January 2015
2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization text January 2018