In this proceeding, we present studies of instrumental systematic effects for the Simons Obsevatory (SO) that are associated with the detector system and its interaction with the full SO experimental systems. SO will measure the Cosmic Microwave Background (CMB) temperature and polarization anisotropies over a wide range of angular scales in six bands with bandcenters spanning from 27 GHz to 270 GHz. We explore effects including intensity-to-polarization leakage due to coupling optics, bolometer nonlinearity, uncalibrated gain variations of bolometers, and readout crosstalk. We model the level of signal contamination, discuss proposed mitigation schemes, and present instrument requirements to inform the design of SO and future CMB projects.

Crowley, K.t., Simon, S.m., Silva-Feaver, M., Goeckner-Wald, N., Ali, A., Austermann, J., et al. (2018). Studies of systematic uncertainties for Simons Observatory: detector array effects. In Proceedings. Millimeter, submillimeter, and far-infrared detectors and instrumentation for astronomy (pp.134). SPIE-INT SOC OPTICAL ENGINEERING [10.1117/12.2313414].

Studies of systematic uncertainties for Simons Observatory: detector array effects

Puglisi, G.;
2018-01-01

Abstract

In this proceeding, we present studies of instrumental systematic effects for the Simons Obsevatory (SO) that are associated with the detector system and its interaction with the full SO experimental systems. SO will measure the Cosmic Microwave Background (CMB) temperature and polarization anisotropies over a wide range of angular scales in six bands with bandcenters spanning from 27 GHz to 270 GHz. We explore effects including intensity-to-polarization leakage due to coupling optics, bolometer nonlinearity, uncalibrated gain variations of bolometers, and readout crosstalk. We model the level of signal contamination, discuss proposed mitigation schemes, and present instrument requirements to inform the design of SO and future CMB projects.
SPIE
Austin, Texas, United States
2018
Rilevanza internazionale
2018
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
detector array; systematic effects; optical coupling; non-linearity; gain variation; crosstalk; Simons Observatory; cosmic microwave background
Intervento a convegno
Crowley, K.t., Simon, S.m., Silva-Feaver, M., Goeckner-Wald, N., Ali, A., Austermann, J., et al. (2018). Studies of systematic uncertainties for Simons Observatory: detector array effects. In Proceedings. Millimeter, submillimeter, and far-infrared detectors and instrumentation for astronomy (pp.134). SPIE-INT SOC OPTICAL ENGINEERING [10.1117/12.2313414].
Crowley, Kt; Simon, Sm; Silva-Feaver, M; Goeckner-Wald, N; Ali, A; Austermann, J; Brown, Ml; Chinone, Y; Cukierman, A; Dober, B; Duff, Sm; Dunkley, J; Errard, J; Fabbian, G; Gallardo, Pa; Ho, S-P; Hubmayr, J; Keating, B; Kusaka, A; Mccallum, N; Mcmahon, J; Nati, F; Niemack, Md; Puglisi, G; Sathyanarayana Rao, M; Reichardt, Cl; Salatino, M; Siritanasak, P; Staggs, S; Suzuki, A; Teply, G; Thomas, Db; Ullom, Jn; Verg(`e)s, C; Vissers, Mr; Westbrook, B; Wollack, Ej; Xu, Z; Zhu, N
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/288200
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