- Abstract:
-
Time-dependent and systematic variations in the band gain and central frequencies of instruments used to study the cosmic microwave background (CMB) are important factors in the data-to-map analysis pipeline. If not properly characterized, they could limit the ability of next-generation experiments to remove astrophysical foreground contamination. Uncertainties include the instrument detector band, which could systematically change across the focal plane, as well as the calibration of the ins...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 2.4mb)
-
- Publisher copy:
- 10.3847/1538-4357/aac71f
-
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- Publisher:
- American Astronomical Society Publisher's website
- Journal:
- Astrophysical Journal Journal website
- Volume:
- 861
- Issue:
- 2
- Pages:
- 82-82
- Publication date:
- 2018-07-06
- Acceptance date:
- 2018-05-20
- DOI:
- EISSN:
-
1538-4357
- ISSN:
-
0004-637X
- Pubs id:
-
pubs:907554
- URN:
-
uri:6882040a-4e53-4473-8fd5-d7c2c155d70b
- UUID:
-
uuid:6882040a-4e53-4473-8fd5-d7c2c155d70b
- Local pid:
- pubs:907554
- Copyright holder:
- American Astronomical Society
- Copyright date:
- 2018
- Notes:
- Copyright © 2018 The American Astronomical Society.
Journal article
The effects of bandpass variations on foreground removal forecasts for future CMB experiments
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