- Abstract:
-
Measurements of cosmic microwave background (CMB) spectral distortions have profound implications for our understanding of physical processes taking place over a vast window in cosmological history. Foreground contamination is unavoidable in such measurements and detailed signal–foreground separation will be necessary to extract cosmological science. In this paper, we present Markov chain Monte Carlo based spectral distortion detection forecasts in the presence of Galactic and extragalactic f...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 3.0MB)
-
- Publisher copy:
- 10.1093/mnras/stx1653
-
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- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 471
- Issue:
- 1
- Pages:
- 1126-1140
- Publication date:
- 2017-06-30
- Acceptance date:
- 2017-06-28
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Pubs id:
-
pubs:922980
- URN:
-
uri:83983dfd-dcb0-4f2c-b7e6-b55457452dd3
- UUID:
-
uuid:83983dfd-dcb0-4f2c-b7e6-b55457452dd3
- Local pid:
- pubs:922980
- Language:
- English
- Keywords:
- Copyright holder:
- Abitbol et al.
- Copyright date:
- 2017
- Notes:
- Copyright © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
Journal article
Prospects for measuring cosmic microwave background spectral distortions in the presence of foregrounds
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