{"paper":{"title":"Planck 2013 results. XI. All-sky model of thermal dust emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Abergel, A. A. Fraisse, A. Beno\\^it, A. Benoit-L\\'evy, A. Bonaldi, A. Catalano, A. Chamballu, A. Coulais, A. Curto, A. De Rosa, A. Gregorio, A. Gruppuso, A. H. Jaffe, A. Hornstrup, A. J. Banday, A. L\\\"ahteenm\\\"aki, A. Lasenby, A. Melchiorri, A. Mennella, A. Moneti, A.-S. Suur-Uski, A. Zacchei, A. Zonca., B. D. Wandelt, B. Maffei, B. P. Crill, B. Rusholme, B. T. Draine, B. Van Tent, C. A. Oxborrow, C. Armitage-Caplan, C. Baccigalupi, C. B. Netterfield, C. Burigana, C. Combet, C. Dickinson, C. Hern\\'andez-Monteagudo, C. Renault, C. R. Lawrence, C. Rosset, D. Hanson, D. Herranz, D. J. Marshall, D. L. Clements, D. L. Harrison, D. Maino, D. Mortlock, D. Munshi, D. Novikov, D. Paoletti, D. Pietrobon, D. Santos, D. Scott, D. Sutton, D. Tavagnacco, D. Yvon, E. Battaner, E. Falgarone, E. Franceschi, E. Hivon, E. Keih\\\"anen, 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. Levrier, 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. Aniano, G. de Zotti, G. Efstathiou, G. Giardino, G. Helou, G. Joncas, 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. A. Grenier, I. Novikov, I. Ristorcelli, J. A. Murphy, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J. Bobin, J. Borrill, J. Delabrouille, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. G. Bartlett, J. Gonz\\'alez-Nuevo, J. J. Bock, J. Jewell, J. Knoche, J. Le\\'on-Tavares, 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. Tuovinen, J. Valiviita, K. Benabed, K. Ganga, K. M. G\\'orski, K. M. Huffenberger, L. A. Wade, L. Danese, L. D. Spencer, L. Knox, L. Mendes, L. Montier, L. Pagano, L. Perotto, L. P. L. Colombo, L. Popa, L. Terenzi, L. Toffolatti, L. Valenziano, L. Verstraete, L.-Y Chiang, M.-A. Miville-Desch\\^enes, M. Arnaud, M. Ashdown, M. Bersanelli, M. Bridges, M. Bucher, M. Clemens, M. Douspis, M. D. Seiffert, M. Frailis, M. Giard, M. Hobson, M. I. R. Alves, M. Juvela, M. Kunz, M. Liguori, M. Linden-V{\\o}rnle, M. L\\'opez-Caniego, M. Maris, M. Massardi, M. Migliaccio, M. Piat, M. Reinecke, M. Remazeilles, M. Rowan-Robinson, M. Sandri, M. Tomasi, M. Tristram, M. Tucci, M. T\\\"urler, N. Aghanim, N. Mandolesi, N. Ponthieu, N. Vittorio, N. Welikala, N. Ysard, O. Dor\\'e, O. Forni, O. Perdereau, P. A. R. Ade, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration, P. Mazzotta, P. McGehee, P. M. Lubin, P. Naselsky, P. Natoli, P. R. Christensen, P. Vielva, R. B. Barreiro, R. C. Butler, R. D. Davies, R. J. Davis, R. J. Laureijs, R. Keskitalo, R. Leonardi, R. Paladini, R.-R. Chary, R. Rebolo, 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, T. A. En{\\ss}lin, T. Ghosh, T. Poutanen, T. Riller, T. R. Jaffe, T. S. Kisner, V. Guillet, V. Stolyarov, W. A. Holmes, W. C. Jones, W. Hovest, W. T. Reach, X. Dupac, Y. Giraud-H\\'eraud","submitted_at":"2013-12-04T19:49:34Z","abstract_excerpt":"This paper presents an all-sky model of dust emission from the Planck 857, 545 and 353 GHz, and IRAS 100 micron data. Using a modified black-body fit to the data we present all-sky maps of the dust optical depth, temperature, and spectral index over the 353-3000 GHz range. This model is a tight representation of the data at 5 arc min. It shows variations of the order of 30 % compared with the widely-used model of Finkbeiner, Davis, and Schlegel. The Planck data allow us to estimate the dust temperature uniformly over the whole sky, providing an improved estimate of the dust optical depth compa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.1300","kind":"arxiv","version":5},"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"}