{"paper":{"title":"Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Blain, A. Bongiovanni, A. Boselli, A. Cava, A. Cimatti, A. Conley, A. Cooray, A. Franceschini, A.J. Smith, A.M.J. Mortier, A.M. Perez Garcia, A. Omont, A. Papageorgiou, A. Poglitsch, A. Saintonge, B. Altieri, B. Maffei, B. Magnelli, B. O'Halloran, B. Schulz, C.D. Dowell, C. Gruppioni, C.K. Xu, C.P. Pearson, D. Burgarella, D. Elbaz, D. Farrah, D.L. Clements, D. Le Borgne, D.L. Shupe, D. Lutz, Douglas Scott, D. Rigopoulou, D. Rizzo, E. Chapin, E. Daddi, E. Dwek, E. Hatziminaoglou, E. Ibar, E. Le Floc'h, E. Sturm, F. Pozzi, G. E. Magdis, G. Lagache, G. Mainetti, G. Rodighiero, G. Wright, H. Aussel, H. Dannerbauer, H. Dominguez, H.M. Lee, H.S. Hwang, H.T. Nguyen, I.G. Roseboom, I. Perez-Fournon, I. Valtchanov, J.A. Stevens, J. Bock, J. Cepa, J.C. Lee, J.D. Vieira, J. Glenn, J.I. Rawlings, J.S. Dunlop, K.E. Tugwell, K. Isaak, K. Okumura, L. Conversi, L. Levenson, L. Marchetti, L. Riguccini, L. Shao, L. Tacconi, L. Vigroux, L.Wang, M. Dickinson, M. Fox, M.G. Lee, M. Griffin, M. Halpern, M.J. Page, M. Pohlen, M. Rowan-Robinson, M. Sanchez Portal, M. Sauvage, M. Symeonidis, M. Trichas, M. Vaccari, M. Zemcov, N. Castro-Rodriguez, N. Forster Schreiber, N. Lu, N. Seymour, P. Andreani, P. Chanial, P. Panuzzo, P. Popesso, P. Santini, R. Auld, R. Genzel, R.J. Ivison, R. Maiolino, R. Nordon, R.-R. Chary, R. Ward, S. Berta, S. Eales, S.J. Oliver, S. Madden, T. Babbedge, V. Arumugam, V. Buat, W. Gear, W.-S. Jeong","submitted_at":"2010-09-06T13:55:32Z","abstract_excerpt":"We study the dust properties of galaxies in the redshift range 0.1<z<2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-North as part of PEP and HerMES key programmes. Infrared (IR) luminosity (L_IR) and dust temperature (T_dust) of galaxies are derived from the spectral energy distribution (SED) fit of the far-infrared (FIR) flux densities obtained with PACS and SPIRE instruments onboard Herschel. As a reference sample, we also obtain IR luminosities and dust temperatures of local galaxies at z<0.1 using AKARI and IRAS data in the field "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.1058","kind":"arxiv","version":1},"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"}