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<i>B</i>-mode polarization forecasts for GreenPol

Abstract:
We present tensor-to-scalar ratio forecasts for GreenPol, a hypothetical ground-based B-mode experiment aiming to survey the cleanest regions of the Northern Galactic hemisphere at five frequencies between 10 and 44 GHz. Its primary science goal would be to measure large-scale CMB polarization fluctuations at multipoles $\ell \lesssim 500$, and thereby constrain the primordial tensor-to-scalar ratio. The observations for the suggested experiment would take place at the Summit Station (72deg N, 38deg W) on Greenland, at an altitude of 3216 meters above sea level. In this paper we simulate various experimental setups, and derive limits on the tensor-to-scalar ratio after CMB component separation using a Bayesian component separation implementation called Commander. When combining the proposed experiment with Planck HFI observations for constraining polarized thermal dust emission, we find a projected limit of r<0.02 at 95 % confidence for the baseline configuration. This limit is very robust with respect to a range of important experimental parameters, including sky coverage, detector weighting, foreground priors etc. Overall, GreenPol would have the possibility to provide deep CMB polarization measurements of the Northern Galactic hemisphere at low frequencies.Comment: 10 pages, 8 figures. To be submitted to A&
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1051/0004-6361/202347393

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Role:
Author
ORCID:
0000-0003-1077-298X
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Role:
Author
ORCID:
0009-0008-0936-6953
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Role:
Author
ORCID:
0000-0003-3821-7275


Publisher:
EDP Sciences
Journal:
Astronomy & Astrophysics More from this journal
Volume:
684
Pages:
A128-A128
Publication date:
2024-02-08
Acceptance date:
2024-01-24
DOI:
EISSN:
1432-0746
ISSN:
0004-6361


Language:
English
Keywords:
Pubs id:
1991305
Local pid:
pubs:1991305
Source identifiers:
W4391658138
Deposit date:
2026-06-10
ARK identifier:
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