Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space mission
Y. Takase, L. Vacher, H. Ishino, G. Patanchon, L. Montier, S. L., Stever, K. Ishizaka, Y. Nagano, W. Wang, J. Aumont, K. Aizawa, A. Anand, C., Baccigalupi, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, S., Basak, M. Bersanelli, M. Bortolami, T. Brinckmann

TL;DR
This paper explores optimal scanning strategies for the LiteBIRD space mission to enhance calibration and systematic effect suppression in measuring the CMB's primordial B-mode polarization, using analytical methods and a new simulation tool.
Contribution
It introduces a comprehensive analytical framework and a fast simulation tool to optimize the scanning strategy for systematic mitigation in the LiteBIRD mission.
Findings
Optimal scanning parameters improve calibration effectiveness.
Certain strategies effectively suppress systematic effects.
Single-detector polarization measurement reduces systematic errors.
Abstract
Large angular scale surveys in the absence of atmosphere are essential for measuring the primordial -mode power spectrum of the Cosmic Microwave Background (CMB). Since this proposed measurement is about three to four orders of magnitude fainter than the temperature anisotropies of the CMB, in-flight calibration of the instruments and active suppression of systematic effects are crucial. We investigate the effect of changing the parameters of the scanning strategy on the in-flight calibration effectiveness, the suppression of the systematic effects themselves, and the ability to distinguish systematic effects by null-tests. Next-generation missions such as LiteBIRD, modulated by a Half-Wave Plate (HWP), will be able to observe polarisation using a single detector, eliminating the need to combine several detectors to measure polarisation, as done in many previous experiments and hence…
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