We quantify the calibration requirements for systematic uncertainties for next-generation ground-based observatories targeting the large-angle B-mode polarization of the Cosmic Microwave Background, with a focus on the Simons Observatory (SO). We explore uncertainties on gain calibration, bandpass center frequencies, and polarization angles, including the frequency variation of the latter across the bandpass. We find that gain calibration and bandpass center frequencies must be known to percent levels or less to avoid biases on the tensor-to-scalar ratio r on the order of Δ r∼10-3, in line with previous findings. Polarization angles must be calibrated to the level of a few tenths of a degree, while their frequency variation between the edges of the band must be known to O(10) degrees. Given the tightness of these calibration requirements, we explore the level to which residual uncertainties on these systematics would affect the final constraints on r if included in the data model and marginalized over. We find that the additional parameter freedom does not degrade the final constraints on r significantly, broadening the error bar by O(10%) at most. We validate these results by reanalyzing the latest publicly available data from the collaboration within an extended parameter space covering both cosmological, foreground and systematic parameters. Finally, our results are discussed in light of the instrument design and calibration studies carried out within SO.

Abitbol, M., Alonso, D., Simon, S., Lashner, J., Crowley, K., Ali, A., et al. (2021). The Simons Observatory: Gain, bandpass and polarization-angle calibration requirements for B-mode searches. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2021(5) [10.1088/1475-7516/2021/05/032].

The Simons Observatory: Gain, bandpass and polarization-angle calibration requirements for B-mode searches

Gabriele Coppi;Valentina Fanfani;Federico Nati;Davide Poletti;Mario Zannoni
2021

Abstract

We quantify the calibration requirements for systematic uncertainties for next-generation ground-based observatories targeting the large-angle B-mode polarization of the Cosmic Microwave Background, with a focus on the Simons Observatory (SO). We explore uncertainties on gain calibration, bandpass center frequencies, and polarization angles, including the frequency variation of the latter across the bandpass. We find that gain calibration and bandpass center frequencies must be known to percent levels or less to avoid biases on the tensor-to-scalar ratio r on the order of Δ r∼10-3, in line with previous findings. Polarization angles must be calibrated to the level of a few tenths of a degree, while their frequency variation between the edges of the band must be known to O(10) degrees. Given the tightness of these calibration requirements, we explore the level to which residual uncertainties on these systematics would affect the final constraints on r if included in the data model and marginalized over. We find that the additional parameter freedom does not degrade the final constraints on r significantly, broadening the error bar by O(10%) at most. We validate these results by reanalyzing the latest publicly available data from the collaboration within an extended parameter space covering both cosmological, foreground and systematic parameters. Finally, our results are discussed in light of the instrument design and calibration studies carried out within SO.
Articolo in rivista - Articolo scientifico
CMBR experiments; CMBR polarization; cosmological parameters from CMBR; gravitational waves and CMBR polarization;
English
13-mag-2021
2021
2021
5
032
none
Abitbol, M., Alonso, D., Simon, S., Lashner, J., Crowley, K., Ali, A., et al. (2021). The Simons Observatory: Gain, bandpass and polarization-angle calibration requirements for B-mode searches. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2021(5) [10.1088/1475-7516/2021/05/032].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/314075
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