Planck2013 results. VIII. HFI photometric calibration and mapmaking

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 29 Oct 2014Embargo end date: 01 Jan 2013 Italy, Spain, Italy, Italy, Denmark, Netherlands, United Kingdom, France, Spain, Italy, France, France, Italy, France, Netherlands, France, Italy, Denmark, Norway, Italy, United Kingdom, France, Ireland, France, France, Italy, Italy, France, United States, United Kingdom, United States, France Publisher:EDP SciencesJournal:Astronomy & Astrophysics, volume 571, page A8 (issn: 0004-6361, eissn: 1432-0746,

Copyright policy )Publicly fundedFunded by:SNSF | Constraining cosmological..., EC | RADIOFOREGROUNDS

Authors: Tauber, Jan; Ade, P. A. R.; Aghanim, N.; Armitage Caplan, C.; Arnaud, M.; Ashdown, M.; Atrio Barandela, F.; +193 Authors

Tauber, Jan; Ade, P. A. R.; Aghanim, N.; Armitage Caplan, C.; Arnaud, M.; Ashdown, M.; Atrio Barandela, F.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Battaner, E.; Benabed, K.; Benoît, A.; Benoit Lévy, A.; Bernard, J. P.; Bersanelli, M.; Bertincourt, B.; Bielewicz, P.; Bobin, J.; Bock, J. J.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bridges, M.; Bucher, M; Burigana, C.; Cardoso, J. F.; Catalano, A.; Challinor, A.; Chamballu, A.; Chary, R. R.; Chen, X.; Chiang, H. C.; Chiang, L. Y.; Christensen, P. R.; Church, S.; Clements, D. L.; Colombi, S.; Colombo, L. P. L.; Combet, C.; Couchot, F.; Coulais, A.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; De Bernardis, P.; De Rosa, A.; De Zotti, G.; Delabrouille, J.; Delouis, J. M.; Désert, F. X.; Dickinson, C.; Diego, J. M.; Dole, H.; Donzelli, S.; Doré, O.; Douspis, M.; Dupac, X.; Efstathiou, G.; Enßlin, T. A.; Eriksen, H. K.; Filliard, C.; Finelli, F.; Forni, O.; Frailis, M.; Franceschi, E.; Galeotta, S.; Ganga, K.; Giard, M.; Giardino, G.; Giraud Héraud, Y.; González Nuevo, J.; Górski, K. M.; Gratton, S.; Gruppuso, A.; Hansen, F. K.; Hanson, D.; Harrison, D.; Helou, G.; Henrot Versillé, S.; Hernández Monteagudo, C.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Hornstrup, A.; Hovest, W.; Huffenberger, K. M.; Jaffe, A. H.; Jaffe, T. R.; Jones, W. C.; Juvela, M.; Keihänen, E.; Keskitalo, R.; Kisner, T. S.; Kneissl, R.; Knoche, J.; Knox, L.; Kunz, M.; Kurki Suonio, H.; Lagache, G.; Lamarre, J. M.; Lasenby, A.; Laureijs, R. J.; Lawrence, C. R.; Le Jeune, M.; Lellouch, E.; Leonardi, R.; Leroy, C.; Lesgourgues, J.; Liguori, M.; Lilje, P. B.; Linden Vørnle, M.; López Caniego, M.; Lubin, P. M.; MacIás Pérez, J. F.; Maffei, B.; Mandolesi, N.; Maris, M.; Marshall, D. J.; Martin, P. G.; Martínez González, E.; Masi, S.; Massardi, M.; Matarrese, S.; Matthai, F.; Maurin, L.; Mazzotta, P.; Mcgehee, P.; Meinhold, P. R.; Melchiorri, A.; Mendes, L.; Mennella, A.; Migliaccio, M.; Mitra, S.; Miville Deschênes, M. A.; Moneti, A.; Montier, L.; Moreno, R.; Morgante, G.; Mortlock, D.; Munshi, D.; Murphy, J. A.; Naselsky, P.; Nati, F.; Natoli, P.; Netterfield, C. B.; Nørgaard Nielsen, H. U.; Noviello, F.; Novikov, D.; Novikov, I.; Osborne, S.; Oxborrow, C. A.; Paci, F.; Pagano, L.; Pajot, F.; Paladini, R.; Paoletti, D.; Partridge, B.; Pasian, F.; Patanchon, G.; Pearson, T. J.; Perdereau, O.; Perotto, L.; Perrotta, F.; Piacentini, F.; Piat, M.; Pierpaoli, E.; Pietrobon, D.; Plaszczynski, S.; Pointecouteau, E.; Polenta, G.; Ponthieu, N.; Popa, L.; Poutanen, T.; Pratt, G. W.; Prézeau, G.; Prunet, S.; Puget, J. L.; Rachen, J. P.; Reinecke, M.; Remazeilles, M.; Renault, C.; Ricciardi, S.; Riller, T.; Ristorcelli, I.; Rocha, G.; Rosset, C.; Roudier, G.; Rusholme, B.; Santos, D.; Savini, G.; Scott, D.; Shellard, E. P. S.; Spencer, L. D.;

doi: 10.1051/0004-6361/201321538 , 10.48550/arxiv.1303.5069

arXiv: 1303.5069

handle: 10261/110566 , 10902/10891 , https://repository.ubn.ru.nl/handle/2066/134819 , 11368/2836135 , 10852/43864 , 2066/134819 , 2434/255110 , 10281/397945 , 11858/00-001M-0000-0025-0343-3 , 11858/00-001M-0000-0025-0341-7 , 11577/3148650 , 2108/177423 , 11573/814393 , 11392/2357550 , 20.500.11767/11628 , 10044/1/60472

Planck2013 results. VIII. HFI photometric calibration and mapmaking

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Abstract

This paper describes the processing applied to the HFI cleaned time-ordered data to produce photometrically calibrated maps. HFI observes the sky over a broad range of frequencies, from 100 to 857 GHz. To get the best accuracy on the calibration on such a large range, two different photometric calibration schemes have to be used. The 545 and 857 \GHz\ data are calibrated using Uranus and Neptune flux density measurements, compared with models of their atmospheric emissions to calibrate the data. The lower frequencies (below 353 GHz) are calibrated using the cosmological microwave background dipole.One of the components of this anisotropy results from the orbital motion of the satellite in the Solar System, and is therefore time-variable. Photometric calibration is thus tightly linked to mapmaking, which also addresses low frequency noise removal. The 2013 released HFI data show some evidence for apparent gain variations of the HFI bolometers' detection chain. These variations were identified by comparing observations taken more than one year apart in the same configuration. We developed an effective correction to limit its effect on calibration, and assess its accuracy. We present several methods used to estimate the precision of the photometric calibration. We distinguish relative (from one detector to another, or from one frequency to another) and absolute uncertainties. In both cases, we found that these uncertainties range from a few $10^{-3}$ to several per cents from 100 to 857 GHz. We describe the pipeline producing the maps from the HFI timelines, based on the photometric calibration parameters and we detail the scheme used to a posteriori set the zero level of the maps. We also briefly discuss the cross-calibration between HFI and the SPIRE instrument on board Herschel. We finally summarize the basic characteristics of the set of the HFI maps from the 2013 Planck data release.

Submitted to Astronomy and Astrophysics. 25 pages, 25 figures, 14 tables. high resolution version available from the ESA website : http://www.sciops.esa.int/index.php?project=PLANCK&page=Planck_Published_Papers (21/01/14) New version with referee's comments resubmitteed to AA

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[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, DIRBE, 1ST DETECTION, cosmic background radiation, Cosmic background radiation, Cosmology: observation, DESIGN, 5107 Particle and high energy physics (for-2020), Survey, 5109 Space sciences (for-2020), 51 Physical Sciences (for-2020), 600, 520, Particle and high energy physics, cosmic background radiation â€“ cosmology: observations â€“ surveys â€“ methods: data analysis, Physical Sciences, astro-ph.CO, Astrophysics - Instrumentation and Methods for Astrophysics, Space Sciences, Astronomical and Space Sciences, Astrophysics - Cosmology and Nongalactic Astrophysics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], astrophysics: cosmology and extragalactic astrophysics; astrophysics: instrumentation and methods for astrophysics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, 0201 Astronomical and Space Sciences (for), Settore FIS/05 - ASTRONOMIA E ASTROFISICA, Astronomy & Astrophysics, 530, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], surveys, PRE-LAUNCH STATUS, DUST EMISSION, Instrumentation and Methods for Astrophysics (astro-ph.IM), ANISOTROPY, [SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 5101 Astronomical sciences (for-2020), SPECTRUM, Science & Technology, Astronomy & Astrophysics (science-metrix), 5109 Space Sciences (for-2020), IN-FLIGHT PERFORMANCE, Astronomy and Astrophysic, Cosmic background radiation; Cosmology: observations; Methods: data analysis; Surveys;, ATMOSPHERE, methods: data analysis, Cosmic background radiation; Cosmology: observations; Methods: data analysis; Surveys; Astronomy and Astrophysics; Space and Planetary Science, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 0201 Astronomical And Space Sciences, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Space and Planetary Science, Cosmic background radiation; Cosmology: observations; Methods: data analysis; Surveys, cosmology: observations, Astronomical sciences, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], COBE FIRAS, [PHYS.ASTR.IM] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], astro-ph.IM, Methods: data analysi

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