Studies of systematic uncertainties for Simons Observatory: Polarization modulator related effects

Maria Salatino, Jacob Lashner, Martina Gerbino, Sara M. Simon, Joy Didier, Aamir Ali, Peter C. Ashton, Sean Bryan, Yuji Chinone, Kevin Coughlin, Kevin T. Crowley, Giulio Fabbian, Nicholas Galitzki, Neil Goeckner-Wald, Jon E. Gudmundsson, Charles A. Hill, Brian Keating, Akito Kusaka, Adrian T. Lee, Jeffrey McMahonAmber D. Miller, Giuseppe Puglisi, Christian L. Reichardt, Grant Teply, Zhilei Xu, Ningfeng Zhu

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

The Simons Observatory (SO) will observe the temperature and polarization anisotropies of the cosmic microwave background (CMB) over a wide range of frequencies (27 to 270 GHz) and angular scales by using both small (â1/40.5 m) and large (â1/46 m) aperture telescopes. The SO small aperture telescopes will target degree angular scales where the primordial B-mode polarization signal is expected to peak. The incoming polarization signal of the small aperture telescopes will be modulated by a cryogenic, continuously-rotating half-wave plate (CRHWP) to mitigate systematic effects arising from slowly varying noise and detector pair-differencing. In this paper, we present an assessment of some systematic effects arising from using a CRHWP in the SO small aperture systems. We focus on systematic effects associated with structural properties of the HWP and effects arising when operating a HWP, including the amplitude of the HWP synchronous signal (HWPSS), and I → P (intensity to polarization) leakage that arises from detector non-linearity in the presence of a large HWPSS. We demonstrate our ability to simulate the impact of the aforementioned systematic effects in the time domain. This important step will inform mitigation strategies and design decisions to ensure that SO will meet its science goals.

Original languageEnglish
Title of host publicationMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
EditorsJonas Zmuidzinas, Jian-Rong Gao
PublisherSPIE
ISBN (Print)9781510619692
DOIs
Publication statusPublished - 2018
EventMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018 - Austin, United States
Duration: 12 Jun 201815 Jun 2018

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume10708

Conference

ConferenceMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018
Country/TerritoryUnited States
CityAustin
Period12/06/1815/06/18

Bibliographical note

Funding Information: This work was supported in part by a grant from the Simons Foundation (Award #457687, B.K.). We would like to thank Tom Essinger-Hileman for many helpful discussions and for making his TMM code publicly available. The authors also acknowledge Julien Peloton for the development of the s4cmb pipeline and his instruction on how to use it. MS acknowledges the financial support of the UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). MG and JEG acknowledge support by the Vetenskapsrådet (Swedish Research Council) through contract No. 638-2013-8993 and the Oskar Klein Centre for Cosmoparticle Physics. Publisher Copyright: © 2018 SPIE.

Other keywords

  • Continuously Rotating Half-Wave Plate
  • Cosmic Microwave Background
  • Intensity to Polarization Leakage
  • Non Linearity
  • Sapphire
  • Simons Observatory
  • Slant Incidence
  • Systematic effects

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