{"paper":{"title":"Planck intermediate results. XLIII. The spectral energy distribution of dust in clusters of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Fraisse, A. Benoit-L\\'evy, A. Bonaldi, A. Catalano, A. Curto, A. De Rosa, A. Ducout, A. Gregorio, A. Gruppuso, A. H. Jaffe, A. Hornstrup, A. L\\\"ahteenm\\\"aki, A. Lasenby, A. Mangilli, A. Melchiorri, A. Mennella, A. Moneti, A. Renzi, A.-S. Suur-Uski, A. Zacchei, A. Zonca, B. Comis, B. Maffei, B. P. Crill, B. Rusholme, C. A. Oxborrow, C. Baccigalupi, C. Burigana, C. Combet, C. Hern\\'andez-Monteagudo, C. Renault, C. R. Lawrence, C. Rosset, D. Herranz, D. L. Harrison, D. Mortlock, D. Munshi, D. Novikov, D. Paoletti, D. Santos, D. Scott, D. Sutton, D. Yvon, E. Battaner, E. Calabrese, E. Churazov, E. Franceschi, E. Gjerl{\\o}w, E. Hivon, E. Keih\\\"anen, E. Mart\\'inez-Gonz\\'alez, E. Pointecouteau, F. Couchot, F. Cuttaia, F. Elsner, F. Finelli, F. K. Hansen, F. Levrier, F. Nati, F. Pajot, F. Pasian, F. Piacentini, F. R. Bouchet, F. Van Tent, F. Villa, F.-X. D\\'esert, G. de Zotti, G. Hurier, G. Lagache, G. Maggio, G. Morgante, G. Polenta, G. Rocha, G. Roudier, G. Savini, G. W. Pratt, H. C. Chiang, H. Dole, H. Kurki-Suonio, H. U. N{\\o}rgaard-Nielsen, I. Bikmaev, I. Khamitov, I. K. Wehus, I. Novikov, I. Ristorcelli, J. A. Murphy, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Delabrouille, J. E. Gudmundsson, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. Gonz\\'alez-Nuevo, J. Knoche, J.-L. Puget, J. M. Diego, J.-M. Lamarre, J. P. Rachen, J. R. Bond, J. Valiviita, K. Benabed, K. Ganga, L. A. Wade, L. Danese, L. Montier, L. Pagano, L. Perotto, L. P. L. Colombo, L. Terenzi, L. Toffolatti, L. Valenziano, M.-A. Miville-Desch\\^enes, M. Ashdown, M. Bersanelli, M. Douspis, M. Frailis, M. Giard, M. Hobson, M. Kunz, M. Lattanzi, M. Liguori, M. Linden-V{\\o}rnle, M. L\\'opez-Caniego, M. Maris, M. Migliaccio, M. Piat, M. Reinecke, M. Remazeilles, M. Rossetti, M. Savelainen, M. Tomasi, M. Tristram, M. Tucci, N. Aghanim, N. Bartolo, N. Mandolesi, N. Ponthieu, O. Dor\\'e, O. Forni, O. Perdereau, P. A. R. Ade, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration: R. Adam, P. Naselsky, P. Natoli, P. R. Christensen, P. Vielva, R. B. Barreiro, R. Burenin, R. J. Davis, R. Keskitalo, R. Kneissl, R. Leonardi, R. Rebolo, R. Stompor, R. Sudiwala, R. Sunyaev, R. T. G\\'enova-Santos, S. Galeotta, S. Masi, S. Matarrese, S. Plaszczynski, S. Prunet, S. R. Hildebrandt, T. A. En{\\ss}lin, T. R. Jaffe, T. S. Kisner, V. Pettorino, V. Stolyarov, W. C. Jones, W. Hovest, X. Dupac, Y. Giraud-H\\'eraud","submitted_at":"2016-03-15T23:06:19Z","abstract_excerpt":"Although infrared (IR) overall dust emission from clusters of galaxies has been statistically detected using data from the Infrared Astronomical Satellite (IRAS), it has not been possible to sample the spectral energy distribution (SED) of this emission over its peak, and thus to break the degeneracy between dust temperature and mass. By complementing the IRAS spectral coverage with Planck satellite data from 100 to 857 GHz, we provide new constraints on the IR spectrum of thermal dust emission in clusters of galaxies. We achieve this by using a stacking approach for a sample of several hundre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.04919","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"}