Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7102
Title: BoloCalc: a sensitivity calculator for the design of Simons Observatory
Authors: Hill, Charles A
Bruno, Sarah Marie M
Sathyanarayana Rao, Mayuri
+ 34 Co-authors
Keywords: CMB
noise
noise-equivalent temperature
mapping speed
sensitivity
Simons Observatory
Issue Date: 2018
Publisher: Society of Photo-Optical Instrumentation Engineers (SPIE)
Citation: Proceedings of the SPIE Vol. 10708, p1070842-1, 2018 , Proceedings of Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX, edited by Jonas Zmuidzinas, Jian-Rong Gao
Abstract: The Simons Observatory (SO) is an upcoming experiment that will study temperature and polarization fluctuations in the cosmic microwave background (CMB) from the Atacama Desert in Chile. SO will field both a large aperture telescope (LAT) and an array of small aperture telescopes (SATs) that will observe in six bands with center frequencies spanning from 27 to 270 GHz. Key considerations during the SO design phase are vast, including the number of cameras per telescope, focal plane magnification and pixel density, in-band optical power and camera throughput, detector parameter tolerances, and scan strategy optimization. To inform the SO design in a rapid, organized, and traceable manner, we have created a Python-based sensitivity calculator with several state-of-the-art features, including detector-to-detector optical white-noise correlations, a handling of simulated and measured bandpasses, and propagation of low-level parameter uncertainties to uncertainty in on-sky noise performance. We discuss the mathematics of the sensitivity calculation, the calculator’s object-oriented structure and key features, how it has informed the design of SO, and how it can enhance instrument design in the broader CMB community, particularly for CMB-S4.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/7102
ISSN: 0277-786X
1996-756X (electronic)
Alternative Location: https://arxiv.org/abs/1806.04316
https://doi.org/10.1117/12.2313916
Copyright: 2018 Society of Photo-Optical Instrumentation Engineers (SPIE)
Appears in Collections:Research Papers (A&A)

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