Studies of systematic uncertainties for Simons Observatory: Detector array effects

التفاصيل البيبلوغرافية
العنوان: Studies of systematic uncertainties for Simons Observatory: Detector array effects
المؤلفون: Crowley K. T., Simon S. M., Silva-Feaver M., Goeckner-Wald N., Ali A., Austermann J., Brown M. L., Chinone Y., Cukierman A., Dober B., Duff S. M., Dunkley J., Errard J., Fabbian G., Gallardo P. A., Ho S. -P. P., Hubmayr J., Keating B., Kusaka A., McCallum N., McMahon J., Nati F., Niemack M. D., Puglisi G., Sathyanarayana Rao M., Reichardt C. L., Salatino M., Siritanasak P., Staggs S., Suzuki A., Teply G., Thomas D. B., Ullom J. N., Verges C., Vissers M. R., Westbrook B., Wollack E. J., Xu Z., Zhu N.
المساهمون: Gao, JR, Crowley, K, Simon, S, Silva-Feaver, M, Goeckner-Wald, N, Ali, A, Austermann, J, Brown, M, Chinone, Y, Cukierman, A, Dober, B, Duff, S, Dunkley, J, Errard, J, Fabbian, G, Gallardo, P, Ho, S, Hubmayr, J, Keating, B, Kusaka, A, Mccallum, N, Mcmahon, J, Nati, F, Niemack, M, Puglisi, G, Sathyanarayana Rao, M, Reichardt, C, Salatino, M, Siritanasak, P, Staggs, S, Suzuki, A, Teply, G, Thomas, D, Ullom, J, Verges, C, Vissers, M, Westbrook, B, Wollack, E, Xu, Z, Zhu, N
بيانات النشر: SPIE
1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA
سنة النشر: 2018
المجموعة: Università degli Studi di Milano-Bicocca: BOA (Bicocca Open Archive)
مصطلحات موضوعية: cosmic microwave background, crosstalk, Detector array, gain variation, non-linearity, optical coupling, Simons Observatory, systematic effects
الوصف: 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.
نوع الوثيقة: conference object
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/isbn/9781510619692; info:eu-repo/semantics/altIdentifier/wos/WOS:000451719300076; ispartofbook:Proceedings of SPIE - The International Society for Optical Engineering; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018; volume:10708; firstpage:134; serie:PROCEEDINGS OF SPIE, THE INTERNATIONAL SOCIETY FOR OPTICAL ENGINEERING; alleditors:Gao, JR; http://hdl.handle.net/10281/247734Test; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85051955439
DOI: 10.1117/12.2313414
الإتاحة: https://doi.org/10.1117/12.2313414Test
http://hdl.handle.net/10281/247734Test
رقم الانضمام: edsbas.444A2CD2
قاعدة البيانات: BASE