Appendix of HFI DPC paper
This page is intented to gather figures that are not inserted in the 2017 DPC paper for readability reasons.
[Section 3.1.2. ]
100 GHz | 143 GHz | 217 GHz | 353 GHz | |
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CO template | ||||
Dust template |
[Complementary of Fig. 11:]
2015 maps | 2017 maps | difference | |||||||
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I | Q | U | I | Q | U | I | Q | U | |
100 GHz | |||||||||
143 GHz | |||||||||
217 GHz | |||||||||
353 GHz | |||||||||
545 GHz | . | . | . | . | . | . | |||
857 GHz | . | . | . | . | . | . |
[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.
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) Delta Cl 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) Delta Cl in rms due to polarization effi?ciency 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) Delta Cl 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.
[Complementary of Fig. 29:]
100 GHz bolometers | 143 GHz bolometers | 217 GHz bolometers | 353 GHz bolometers | ||||
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[Complementary of Fig. 47:]
Data Processing Center
EMI/EMC influence of the 4K cooler mechanical motion on the bolometer readout electronics.
analog to digital converter