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Sensitivity modeling for LiteBIRD

Abstract:
LiteBIRD is a future satellite mission designed to observe the polarization of the cosmic microwave background radiation in order to probe the inflationary universe. LiteBIRD is set to observe the sky using three telescopes with transition-edge sensor bolometers. In this work we estimated the LiteBIRD instrumental sensitivity using its current design. We estimated the detector noise due to the optical loadings using physical optics and ray-tracing simulations. The noise terms associated with thermal carrier and readout noise were modeled in the detector noise calculation. We calculated the observational sensitivities over fifteen bands designed for the LiteBIRD telescopes using assumed observation time efficiency.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1007/s10909-022-02921-7

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Christ Church
Role:
Author
ORCID:
0000-0002-4598-9719


More from this funder
Funder identifier:
https://ror.org/057g20z61
Grant:
ST/W000903/1
ST/P004474/2
More from this funder
Funder identifier:
https://ror.org/005ta0471


Publisher:
Springer Nature
Journal:
Journal of Low Temperature Physics More from this journal
Volume:
211
Issue:
5-6
Pages:
384-397
Publication date:
2022-12-02
Acceptance date:
2022-11-01
DOI:
EISSN:
1573-7357
ISSN:
0022-2291


Language:
English
Keywords:
Pubs id:
1314665
Local pid:
pubs:1314665
Deposit date:
2025-05-07

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