Appendix of HFI DPC paper

This page is intented to gather figures that are not inserted in the 2017 DPC paper for readability reasons.

[Complementary of Fig. 44:]

Comparaison of 2015 and 2017 I, Q and U maps and their difference.

	2015 maps			2017 maps			difference
	I	Q	U	I	Q	U	I	Q	U
100 GHz	File:100GHz DX11 I.pdf	File:100GHz DX11 Q.pdf	File:100GHz DX11 U.pdf		File:100GHz Q.pdf.pdf	File:100GHz U.pdf.pdf
143 GHz				File:143GHz I.pdf.pdf	File:143GHz Q.pdf.pdf	File:143GHz U.pdf.pdf
217 GHz				File:217GHz I.pdf.pdf	File:217GHz Q.pdf.pdf	File:217GHz U.pdf.pdf
353 GHz				File:353GHz I.pdf.pdf	File:353GHz Q.pdf.pdf	File:353GHz U.pdf.pdf
545 GHz		.	.	File:545GHz I.pdf.pdf	.	.		.	.
857 GHz		.	.	File:857GHz I.pdf.pdf	.	.		.	.

[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. 20:]

Map and power spectra from E2E simulations difference with and without 4K lines.

100 GHz bolometers		143 GHz bolometers		217 GHz bolometers		353 GHz bolometers
.	.
.	.
.	.
.	.	.	.

[Complementary of Fig. 38:]

ADCNL induced gain time variation as a function of ring numbers. Blue line shows the solved gain variation for the data and grey ones show 10 realizations drawn within the uncertainties of the ADC model.

100 GHz bolometers	143 GHz bolometers	217 GHz bolometers	353 GHz bolometers