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The Simons Observatory: science goals and forecasts

Abstract:

The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experiment, motivate the design, and forecast its performance. SO will measure the temperature and polarization anisotropy of the cosmic microwave background in six frequency bands centered at: 27, 39, 93, 145, 225 and 280 GHz. The initial configuration of SO will have three small-aperture 0.5-m te...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1475-7516/2019/02/056

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0002-4598-9719
Publisher:
IOP Publishing Publisher's website
Journal:
Journal of Cosmology and Astroparticle Physics Journal website
Volume:
2019
Article number:
056
Publication date:
2019-02-27
Acceptance date:
2019-01-14
DOI:
EISSN:
1475-7516
Language:
English
Keywords:
Pubs id:
pubs:953603
UUID:
uuid:3cf90506-4fb9-4ec7-84a4-1c17a3557757
Local pid:
pubs:953603
Source identifiers:
953603
Deposit date:
2019-04-11

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