{"paper":{"title":"Planck 2013 results. VIII. HFI photometric calibration and mapmaking","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"A. Beno\\^it, A. Benoit-L\\'evy, A. Catalano, A. Challinor, A. Chamballu, A. Coulais, A. Curto, A. De Rosa, A. Gregorio, A. Gruppuso, A. H. Jaffe, A. Hornstrup, A. J. Banday, A. Lasenby, A. Melchiorri, A. Mennella, A. Moneti, A.-S. Suur-Uski, A. Zacchei, A. Zonca, B. Bertincourt, B. D. Wandelt, B. Maffei, B. Partridge, B. P. Crill, B. Rusholme, B. Van Tent, C. A. Oxborrow, C. Armitage-Caplan, C. Baccigalupi, C. B. Netterfield, C. Burigana, C. Combet, C. Dickinson, C. Filliard, C. Hern\\'andez-Monteagudo, C. Leroy, C. Renault, C. R. Lawrence, C. Rosset, D. Hanson, D. Harrison, D. Herranz, D. J. Marshall, D. L. Clements, D. Mortlock, D. Munshi, D. Novikov, D. Paoletti, D. Pietrobon, D. Santos, D. Sutton, D. Tavagnacco, D. Yvon, E. Battaner, E. Franceschi, E. Hivon, E. Keih\\\"anen, E. Lellouch, E. Mart\\'inez-Gonz\\'alez, E. Pierpaoli, E. Pointecouteau, E. P. S. Shellard, F. Atrio-Barandela, F. Boulanger, F. Couchot, F. Cuttaia, F. Finelli, F. K. Hansen, F. Matthai, F. Nati, F. Noviello, F. Paci, F. Pajot, F. Pasian, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Sureau, F. Villa, F.-X. D\\'esert, G. de Zotti, G. Efstathiou, G. Giardino, G. Helou, G. Lagache, G. Morgante, G. Patanchon, G. Polenta, G. Pr\\'ezeau, G. Rocha, G. Roudier, G. Savini, G. Umana, G. W. Pratt, H. C. Chiang, H. Dole, H. K. Eriksen, H. Kurki-Suonio, H. U. N{\\o}rgaard-Nielsen, I. Novikov, I. Ristorcelli, J. A. Murphy, J. A. Tauber, J. Aumont, J. Bobin, J. Borrill, J. Delabrouille, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. Gonz\\'alez-Nuevo, J. J. Bock, J. Knoche, J. Lesgourgues, J.-L. Puget, J.-L. Starck, J.-M. Delouis, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Valiviita, K. Benabed, K. Ganga, K. M. G\\'orski, K. M. Huffenberger, L. A. Wade, L. Danese, L. D. Spencer, L. Knox, L. Maurin, L. Mendes, L. Montier, L. Pagano, L. Perotto, L. P. L. Colombo, L. Popa, L. Terenzi, L. Valenziano, L.-Y Chiang, M.-A. Miville-Desch\\^enes, M. Arnaud, M. Ashdown, M. Bersanelli, M. Bridges, M. Bucher, M. Douspis, M. Frailis, M. Giard, M. Hobson, M. Juvela, M. Kunz, M. Le Jeune, M. Liguori, M. Linden-V{\\o}rnle, M. L\\'opez-Caniego, M. Maris, M. Migliaccio, M. Piat, M. Reinecke, M. Remazeilles, M. Tomasi, M. Tristram, M. Tucci, N. Aghanim, N. Mandolesi, N. Ponthieu, N. Vittorio, O. Dor\\'e, O. Forni, O. Perdereau, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration: P. A. R. Ade, P. Mazzotta, P. McGehee, P. M. Lubin, P. Naselsky, P. Natoli, P. R. Christensen, P. R. Meinhold, P. Vielva, R. B. Barreiro, R. D. Davies, R. J. Laureijs, R. Keskitalo, R. Kneissl, R. Leonardi, R. Moreno, R. Paladini, R.-R. Chary, R. Stompor, R. Sudiwala, R. Sunyaev, S. Church, S. Colombi, S. Donzelli, S. Galeotta, S. Gratton, S. Henrot-Versill\\'e, S. Masi, S. Matarrese, S. Mitra, S. Osborne, S. Plaszczynski, S. Prunet, S. R. Hildebrandt, S. Ricciardi, S. Techene, T. A. En{\\ss}lin, T. Poutanen, T. Riller, T. R. Jaffe, T. S. Kisner, V. Stolyarov, W. A. Holmes, W. C. Jones, W. Hovest, X. Chen, X. Dupac, Y. Giraud-H\\'eraud","submitted_at":"2013-03-20T20:10:08Z","abstract_excerpt":"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 di"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.5069","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}