Appendix of HFI DPC paper
This page is intented to provide complementary figures to those of the 2017 HFI DPC paper (Planck-2020-A3[1]).
Section 5.3.10: for convenience, we reproduce here Figures 6, 7 and 8 of Rosset et al.
This paper is published as Rosset et al. Planck pre-launch status: High Frequency Instrument polarization calibration. 2010b, A&A, 520, A13 Planck-PreLaunch-XIII[2]. The figures 6, 7 et 8 reproduced hereunder are given in the version on ArXiv 1004.2595
gain errors (1) | polarization efficiency errors (2) | orientation errors (3) |
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(1)
in rms due to gain errors from 0.01% to 1% for E-mode (top) and B-mode (bottom) compared to initial spectrum (solid black lines). Cosmic variance for E-mode is plotted in dashed black line.(2)
in rms due to polarization efficiency errors from 0.1% to 4% for E-mode (top) and B-mode (bottom) compared to initial spectrum (solid black lines). Cosmic variance for E-mode is plotted in dashed black line.(3)
in rms due to various orientation errors from 0.25 to 2 degrees for E-mode (top) and B-mode (bottom) compared to initial spectrum (solid black lines). Cosmic variance for E-mode is plotted in dashed black line.Section 5.5: complementary figures of Fig. 29
100 GHz bolometers | 143 GHz bolometers | 217 GHz bolometers | 353 GHz bolometers | ||||
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Section 5.13: complementary figures of Fig. 47
References[edit]
- ↑ Planck 2018 results. III. High Frequency Instrument data processing and frequency maps, Planck Collaboration, 2020, A&A, 641, A3.
- ↑ Planck pre-launch status: High Frequency Instrument polarization calibration, C. Rosset, M. Tristram, N. Ponthieu, et al. , A&A, 520, A13+, (2010).
(Planck) High Frequency Instrument
Data Processing Center
EMI/EMC influence of the 4K cooler mechanical motion on the bolometer readout electronics.
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