{"paper":{"title":"Planck Early Results XXIV: Dust in the diffuse interstellar medium and the Galactic halo","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Balbi, A. Benoit, A. Bonaldi, A. Catalano, A. Challinor, A. Chamballu, A. Coulais, A. De Rosa, A. Gregorio, A. Gruppuso, A. H. Jaffe, A. J. Banday, A. Jones, A. Lasenby, A. Melchiorri, A. Mennella, A. Moneti, A. Murphy, A. Wilkinson, A. Zacchei, A. Zonca, B. D. Wandelt, B. Maffei, B. P. Crill, B. Rusholme, C. Baccigalupi, C. B. Netterfield, C. Burigana, C. Chiang, C. Dickinson, C. J. MacTavish, C. Leroy, C. M. Cantalupo, C. Renault, C. R. Lawrence, C. Rosset, D. Harrison, D. Herranz, D. J. Marshall, D. L. Clements, D. Maino, D. Mortlock, D. Munshi, D. Novikov, D. Pinheiro Goncalves, D. Santos, D. Scott, D. Yvon, E. Battaner, E. Franceschi, E. Hivon, E. Keihanen, E. Martinez-Gonzalez, E. Pointecouteau, F. Boulanger, F. Couchot, F. Cuttaia, F. Finelli, F. J. Lockman, F. K. Hansen, F. Matthai, F. Nati, F. Noviello, F. Pajot, F. Pasian, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Stivoli, F. Villa, F.-X. Desert, G. De Gasperis, G. de Zotti, G. Efstathiou, G. F. Smoot, G. Giardino, G. Helou, G. Joncas, G. Lagache, G. Morgante, G. Patanchon, G. Polenta, G. Prezeau, G. Rocha, G. Savini, G. Umana, H. K. Eriksen, H. Kurki-Suonio, H. U. Norgaard-Nielsen, I. J. O'Dwyer, I. Novikov, I. Ristorcelli, J. A. Rubino-Martin, J. A. Tauber, J. Aumont, J. Borrill, J. Delabrouille, J.-F. Cardoso, J. F. Macias-Perez, J.-F. Sygnet, J. G. Bartlett, J. Gonzalez-Nuevo, J. J. Bock, J.-L. Puget, J.-L. Starck, J.-M. Delouis, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J.-P. Torre, J. R. Bond, J. Tuovinen, K. Benabed, K. Blagrave, K. Ganga, K. M. Gorski, K. M. Huffenberger, L. A. Wade, L. Cayon, L. Danese, L. Knox, L. Mendes, L. Montier, L. Perotto, L. Terenzi, L. Toffolatti, L. Valenziano, L.-Y Chiang, M.-A. Miville-Deschenes, M. Arnaud, M. Ashdown, M. Bersanelli, M. Bucher, M. Douspis, M. D. Seiffert, M. Frailis, M. Giard, M. Hobson, M. Juvela, M. Linden-Vornle, M. Lopez-Caniego, M. Maris, M. Piat, M. Reinecke, M. Rowan-Robinson, M. Sandri, M. Tomasi, M. Tristram, N. Aghanim, N. Mandolesi, N. Ponthieu, N. Vittorio, O. Dore, O. Forni, O. Perdereau, P. A. R. Ade, P. Cabella, P. De Bernardis, Planck Collaboration: A. Abergel, P. Martin, P. Mazzotta, P. McGehee, P. M. Lubin, P. Naselsky, P. Natoli, P. R. Christensen, P. R. Meinhold, P. Shellard, P. Vielva, R. B. Barreiro, R. Bhatia, R. D. Davies, R. J. Davis, R. J. Hoyland, R. J. Laureijs, R. Keskitalo, R. Kneissl, R. Leonardi, R. Mann, R. Paladini, R. Stompor, R. Sudiwala, S. Colombi, S. Donzelli, S. Galeotta, S. Gratton, S. Henrot-Versille, S. Leach, S. Masi, S. Matarrese, S. Osborne, S. Plaszczynski, S. Prunet, S. R. Hildebrandt, S. Ricciardi, T. A. Ensslin, T. Poutanen, T. Riller, T. S. Kisner, U. Dorl, V. Stolyarov, W. A. Holmes, W. C. Jones, W. Hovest, W. T. Reach, X. Dupac, Y. Giraud-Heraud","submitted_at":"2011-01-11T18:41:21Z","abstract_excerpt":"This paper presents the first results of comparison of Planck along with IRAS data with Green Bank Telescope 21-cm observations in 14 fields covering more than 800 square degrees at high Galactic latitude. Galactic dust emission for fields with average HI column density lower than 2 x 10^20 cm^-2 is well correlated with 21-cm emission. The residual emission in these fields, once the HI-correlated emission is removed, is consistent with the expected statistical properties of the cosmic infrared background fluctuations. Fields with larger column densities show significant excess dust emission co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.2036","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"}