{"paper":{"title":"Herschel unveils a puzzling uniformity of distant dusty galaxies","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 Garc{\\i}a, 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.Daddi, E.Dwek, E.Hatziminaoglou, E.Ibar, E.Le Floc'h, E.Sturm, F.Pozzi, G.Lagache, G.Magdis, G.Mainetti, G.Rodighiero, G.Wright, H.Aussel, H.Dominguez, H.S.Hwang, H.T.Nguyen, I.G.Roseboom, I.Perez Fournon, I.Valtchanov, J.A.Stevens, J.Bock, J.Cepa, J.Glenn, J.I.Rawlings, J.S.Dunlop, J.Vieira, 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.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","submitted_at":"2010-05-17T09:58:51Z","abstract_excerpt":"The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the spectral energy distribution (SED) and dust temperature of galaxies have strongly evolved since z~2.5. We use Herschel deep extragalactic surveys from 100 to 500um to compute total IR luminosities in galaxies down to the faintest levels, using PACS and SPIRE in the GOODS-North field (PEP and HerMES key programs). We show that measurements in the SPIRE bands can "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.2859","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"}