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dc.date.accessioned2017-05-03T13:12:16Z
dc.date.available2017-05-03T13:12:16Z
dc.date.created2017-01-28T19:19:54Z
dc.date.issued2016
dc.identifier.citationAdam, R. Ade, P. A. R. Aghanim, N. Ashdown, M. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartolo, N. Battaner, E. Benabed, K. Benoit-Lévy, A. Bersanelli, M. Bielewicz, P. Bikmaev, I. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Burenin, R. Burigana, C. Calabrese, E. Cardoso, J.-F. Catalano, A. Chiang, H. C. Christensen, P. R. Churazov, E. Colombo, L. P. L. Combet, C. Comis, B. Couchot, F. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Désert, F.-X. Diego, J. M. Dole, H. Doré, O. Douspis, M. Ducout, A. Dupac, X. Elsner, F. Enßlin, T. A. Finelli, F. Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Ganga, K Genova-Santos, RT Giard, M Giraud-Heraud, Y Gjerløw, Eirik Gonzalez-Nuevo, J Gorski, KM Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, Frode Kristian Harrison, DL Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Hornstrup, A Hovest, W Hurier, G Jaffe, AH Jaffe, TR Jones, WC Keihänen, E Keskitalo, R Khamitov, I Kisner, TS Kneissl, R Knoche, J Kunz, M Kurki-Suonio, H Lagache, G Lähteenmäki, A Lamarre, JM Lasenby, A Lattanzi, M Lawrence, CR Leonardi, R Levrier, F Liguori, M Lilje, Per Barth Linden-Vørnle, M Lopez-Caniego, M Macias-Perez, JF Maffei, B Maggio, G Mandolesi, N Mangilli, A Maris, M Martin, PG Martinez-Gonzalez, E Masi, S Matarrese, S Melchiorri, A Mennella, A Migliaccio, M Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Nørgaard-Nielsen, HU Novikov, D Novikov, I Oxborrow, CA Pagano, L Pajot, F Paoletti, D Pasian, F Perdereau, O Perotto, L Pettorino, V Piacentini, F Piat, M Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Pratt, GW Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Renault, C Renzi, A Ristorcelli, I Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Santos, D Savelainen, M Savini, G Scott, D Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Valenziano, L Valiviita, J Van Tent, F Vielva, P Villa, F Wade, LA Wehus, Ingunn Kathrine Yvon, D Zacchei, A Zonca, A . Planck intermediate results: XLIII. Spectral energy distribution of dust in clusters of galaxies. Astronomy and Astrophysics. 2016, 596
dc.identifier.urihttp://hdl.handle.net/10852/55324
dc.description.abstractAlthough 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 hundred objects from the Planck cluster sample. This procedure averages out fluctuations from the IR sky, allowing us to reach a significant detection of the faint cluster contribution. We also use the large frequency range probed by Planck, together with component-separation techniques, to remove the contamination from both cosmic microwave background anisotropies and the thermal Sunyaev-Zeldovich effect (tSZ) signal, which dominate at ν ≤ 353 GHz. By excluding dominant spurious signals or systematic effects, averaged detections are reported at frequencies 353 GHz ≤ ν ≤ 5000 GHz. We confirm the presence of dust in clusters of galaxies at low and intermediate redshifts, yielding an SED with a shape similar to that of the Milky Way. Planck’s resolution does not allow us to investigate the detailed spatial distribution of this emission (e.g. whether it comes from intergalactic dust or simply the dust content of the cluster galaxies), but the radial distribution of the emission appears to follow that of the stacked SZ signal, and thus the extent of the clusters. The recovered SED allows us to constrain the dust mass responsible for the signal and its temperature.en_US
dc.languageEN
dc.publisherEDP Sciences
dc.titlePlanck intermediate results: XLIII. Spectral energy distribution of dust in clusters of galaxiesen_US
dc.typeJournal articleen_US
dc.creator.authorAdam, R.
dc.creator.authorAde, P. A. R.
dc.creator.authorAghanim, N.
dc.creator.authorAshdown, M.
dc.creator.authorAumont, J.
dc.creator.authorBaccigalupi, C.
dc.creator.authorBanday, A. J.
dc.creator.authorBarreiro, R. B.
dc.creator.authorBartolo, N.
dc.creator.authorBattaner, E.
dc.creator.authorBenabed, K.
dc.creator.authorBenoit-Lévy, A.
dc.creator.authorBersanelli, M.
dc.creator.authorBielewicz, P.
dc.creator.authorBikmaev, I.
dc.creator.authorBonaldi, A.
dc.creator.authorBond, J. R.
dc.creator.authorBorrill, J.
dc.creator.authorBouchet, F. R.
dc.creator.authorBurenin, R.
dc.creator.authorBurigana, C.
dc.creator.authorCalabrese, E.
dc.creator.authorCardoso, J.-F.
dc.creator.authorCatalano, A.
dc.creator.authorChiang, H. C.
dc.creator.authorChristensen, P. R.
dc.creator.authorChurazov, E.
dc.creator.authorColombo, L. P. L.
dc.creator.authorCombet, C.
dc.creator.authorComis, B.
dc.creator.authorCouchot, F.
dc.creator.authorCrill, B. P.
dc.creator.authorCurto, A.
dc.creator.authorCuttaia, F.
dc.creator.authorDanese, L.
dc.creator.authorDavis, R. J.
dc.creator.authorde Bernardis, P.
dc.creator.authorde Rosa, A.
dc.creator.authorde Zotti, G.
dc.creator.authorDelabrouille, J.
dc.creator.authorDésert, F.-X.
dc.creator.authorDiego, J. M.
dc.creator.authorDole, H.
dc.creator.authorDoré, O.
dc.creator.authorDouspis, M.
dc.creator.authorDucout, A.
dc.creator.authorDupac, X.
dc.creator.authorElsner, F.
dc.creator.authorEnßlin, T. A.
dc.creator.authorFinelli, F.
dc.creator.authorForni, O
dc.creator.authorFrailis, M
dc.creator.authorFraisse, AA
dc.creator.authorFranceschi, E
dc.creator.authorGaleotta, S
dc.creator.authorGanga, K
dc.creator.authorGenova-Santos, RT
dc.creator.authorGiard, M
dc.creator.authorGiraud-Heraud, Y
dc.creator.authorGjerløw, Eirik
dc.creator.authorGonzalez-Nuevo, J
dc.creator.authorGorski, KM
dc.creator.authorGregorio, A
dc.creator.authorGruppuso, A
dc.creator.authorGudmundsson, JE
dc.creator.authorHansen, Frode Kristian
dc.creator.authorHarrison, DL
dc.creator.authorHernandez-Monteagudo, C
dc.creator.authorHerranz, D
dc.creator.authorHildebrandt, SR
dc.creator.authorHivon, E
dc.creator.authorHobson, M
dc.creator.authorHornstrup, A
dc.creator.authorHovest, W
dc.creator.authorHurier, G
dc.creator.authorJaffe, AH
dc.creator.authorJaffe, TR
dc.creator.authorJones, WC
dc.creator.authorKeihänen, E
dc.creator.authorKeskitalo, R
dc.creator.authorKhamitov, I
dc.creator.authorKisner, TS
dc.creator.authorKneissl, R
dc.creator.authorKnoche, J
dc.creator.authorKunz, M
dc.creator.authorKurki-Suonio, H
dc.creator.authorLagache, G
dc.creator.authorLähteenmäki, A
dc.creator.authorLamarre, JM
dc.creator.authorLasenby, A
dc.creator.authorLattanzi, M
dc.creator.authorLawrence, CR
dc.creator.authorLeonardi, R
dc.creator.authorLevrier, F
dc.creator.authorLiguori, M
dc.creator.authorLilje, Per Barth
dc.creator.authorLinden-Vørnle, M
dc.creator.authorLopez-Caniego, M
dc.creator.authorMacias-Perez, JF
dc.creator.authorMaffei, B
dc.creator.authorMaggio, G
dc.creator.authorMandolesi, N
dc.creator.authorMangilli, A
dc.creator.authorMaris, M
dc.creator.authorMartin, PG
dc.creator.authorMartinez-Gonzalez, E
dc.creator.authorMasi, S
dc.creator.authorMatarrese, S
dc.creator.authorMelchiorri, A
dc.creator.authorMennella, A
dc.creator.authorMigliaccio, M
dc.creator.authorMiville-Deschenes, MA
dc.creator.authorMoneti, A
dc.creator.authorMontier, L
dc.creator.authorMorgante, G
dc.creator.authorMortlock, D
dc.creator.authorMunshi, D
dc.creator.authorMurphy, JA
dc.creator.authorNaselsky, P
dc.creator.authorNati, F
dc.creator.authorNatoli, P
dc.creator.authorNørgaard-Nielsen, HU
dc.creator.authorNovikov, D
dc.creator.authorNovikov, I
dc.creator.authorOxborrow, CA
dc.creator.authorPagano, L
dc.creator.authorPajot, F
dc.creator.authorPaoletti, D
dc.creator.authorPasian, F
dc.creator.authorPerdereau, O
dc.creator.authorPerotto, L
dc.creator.authorPettorino, V
dc.creator.authorPiacentini, F
dc.creator.authorPiat, M
dc.creator.authorPlaszczynski, S
dc.creator.authorPointecouteau, E
dc.creator.authorPolenta, G
dc.creator.authorPonthieu, N
dc.creator.authorPratt, GW
dc.creator.authorPrunet, S
dc.creator.authorPuget, JL
dc.creator.authorRachen, JP
dc.creator.authorRebolo, R
dc.creator.authorReinecke, M
dc.creator.authorRemazeilles, M
dc.creator.authorRenault, C
dc.creator.authorRenzi, A
dc.creator.authorRistorcelli, I
dc.creator.authorRocha, G
dc.creator.authorRosset, C
dc.creator.authorRossetti, M
dc.creator.authorRoudier, G
dc.creator.authorRubino-Martin, JA
dc.creator.authorRusholme, B
dc.creator.authorSantos, D
dc.creator.authorSavelainen, M
dc.creator.authorSavini, G
dc.creator.authorScott, D
dc.creator.authorStolyarov, V
dc.creator.authorStompor, R
dc.creator.authorSudiwala, R
dc.creator.authorSunyaev, R
dc.creator.authorSutton, D
dc.creator.authorSuur-Uski, AS
dc.creator.authorSygnet, JF
dc.creator.authorTauber, JA
dc.creator.authorTerenzi, L
dc.creator.authorToffolatti, L
dc.creator.authorTomasi, M
dc.creator.authorTristram, M
dc.creator.authorTucci, M
dc.creator.authorValenziano, L
dc.creator.authorValiviita, J
dc.creator.authorVan Tent, F
dc.creator.authorVielva, P
dc.creator.authorVilla, F
dc.creator.authorWade, LA
dc.creator.authorWehus, Ingunn Kathrine
dc.creator.authorYvon, D
dc.creator.authorZacchei, A
dc.creator.authorZonca, A
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1440028
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy and Astrophysics&rft.volume=596&rft.spage=&rft.date=2016
dc.identifier.jtitleAstronomy and Astrophysics
dc.identifier.volume596
dc.identifier.pagecount12
dc.identifier.doihttp://dx.doi.org/10.1051/0004-6361/201628522
dc.identifier.urnURN:NBN:no-58115
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-6361
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/55324/2/Intermediate_XLIII.pdf
dc.type.versionPublishedVersion
cristin.articleidA104


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