B-mode polarization forecasts for GreenPol

• Published in: Astronomy & Astrophysics
• Main Authors: Fuskeland, Unni, Kaplan, A., Wehus, Ingunn Kathrine, Eriksen, Hans Kristian Kamfjord, Christensen, P.R., von Hausegger, S., Liu, H., Lubin, P.M., Meinhold, P.R., Naselsky, P., Thommesen, Harald, Zonca, A.
• Format: Article in Journal/Newspaper
• Language: English
• Published: 2024
• Subjects: VDP::Astrofysikk; astronomi: 438; Greenland
• Online Access: http://hdl.handle.net/10852/111216; https://doi.org/10.1051/0004-6361/202347393

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 cosmic microwave background (CMB) polarization fluctuations at multipoles ℓ ≲ 500, and thereby constrain the primordial tensor-to-scalar ratio r. The observations for the suggested experiment would take place at the Summit Station (72 ° 34N, 38 ° 27W) on Greenland, at an altitude of 3216 m above sea level. For this paper we simulated various experimental setups, and derived 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 found 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, among others. Overall, GreenPol would have the possibility to provide deep CMB polarization measurements of the Northern Galactic Hemisphere at low frequencies.