001596584 001__ 1596584
001596584 003__ SzGeCERN
001596584 005__ 20210503223237.0
001596584 0247_ $$2DOI$$a10.1051/0004-6361/201322093
001596584 0248_ $$aoai:cds.cern.ch:1596584$$qcerncds:CERN
001596584 037__ $$aarXiv:1309.0382
001596584 035__ $$9arXiv$$aoai:arXiv.org:1309.0382$$d2015-06-17$$h2015-06-26T08:36:45Z$$m$$ttrue$$uhttp://export.arxiv.org/oai2
001596584 035__ $$9Inspire$$a1252033
001596584 041__ $$aeng
001596584 100__ $$aAde, P A R
001596584 245__ $$aPlanck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
001596584 269__ $$c02 Sep 2013
001596584 260__ $$c2014
001596584 300__ $$a39 p
001596584 500__ $$9arXiv$$a
001596584 520__ $$aWe present new measurements of CIB anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross frequency power spectrum is measured from 143 to 3000 GHz, and the auto-bispectrum from 217 to 545 GHz. The total areas used to compute the CIB power spectrum and bispectrum are about 2240 and 4400 deg^2, respectively. After careful removal of the contaminants, and a complete study of systematics, the CIB power spectrum and bispectrum are measured with unprecedented signal to noise ratio from angular multipoles ell~150 to 2500, and ell~130 to 1100, respectively. Two approaches are developed for modelling CIB power spectrum anisotropies. The first approach takes advantage of the unique measurements by Planck at large angular scales, and models only the linear part of the power spectrum, with a mean bias of dark matter halos hosting dusty galaxies at a given redshift weighted by their contribution to the emissivities. The second approach is based on a model that associates star-forming galaxies with dark matter halos and their subhalos, using a parametrized relation between the dust-processed infrared luminosity and (sub-)halo mass. The two approaches simultaneously fit all auto- and cross- power spectra very well. We find that the star formation history is well constrained up to z~2. However, at higher redshift, the accuracy of the star formation history measurement is strongly degraded by the uncertainty in the spectral energy distribution of CIB galaxies. We also find that CIB galaxies have warmer temperatures as redshift increases. The CIB bispectrum is steeper than that expected from the power spectrum, although well fitted by a power law; this gives some information about the contribution of massive halos to the CIB bispectrum.
001596584 540__ $$aarXiv nonexclusive-distrib. 1.0$$barXiv$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
001596584 595__ $$agiva a faire
001596584 595__ $$aLANL EDS
001596584 595__ $$aNot for annual report
001596584 595__ $$aNot CERN
001596584 595__ $$aCDS
001596584 595__ $$aNot for annual report
001596584 65017 $$2arXiv$$aAstrophysics and Astronomy
001596584 690C_ $$aARTICLE
001596584 695__ $$9LANL EDS$$aastro-ph.CO
001596584 693__ $$ePLANCK RE24
001596584 700__ $$aAghanim, N
001596584 700__ $$aArmitage-Caplan, C
001596584 700__ $$aArnaud, M
001596584 700__ $$aAshdown, M
001596584 700__ $$aAtrio-Barandela, F
001596584 700__ $$aAumont, J
001596584 700__ $$0AUTHOR|(CDS)2087245$$9#BEARD#$$aBaccigalupi, C
001596584 700__ $$aBanday, A J
001596584 700__ $$aBarreiro, R B
001596584 700__ $$aBartlett, J G
001596584 700__ $$aBattaner, E
001596584 700__ $$aBenabed, K
001596584 700__ $$aBenoît, A
001596584 700__ $$aBenoit-Lévy, A
001596584 700__ $$aBernard, J -P
001596584 700__ $$aBersanelli, M
001596584 700__ $$aBethermin, M
001596584 700__ $$aBielewicz, P
001596584 700__ $$aBlagrave, K
001596584 700__ $$aBobin, J
001596584 700__ $$aBock, J J
001596584 700__ $$aBonaldi, A
001596584 700__ $$aBond, J R
001596584 700__ $$aBorrill, J
001596584 700__ $$aBouchet, F R
001596584 700__ $$aBoulanger, F
001596584 700__ $$aBridges, M
001596584 700__ $$aBucher, M
001596584 700__ $$aBurigana, C
001596584 700__ $$aButler, R C
001596584 700__ $$aCardoso, J -F
001596584 700__ $$aCatalano, A
001596584 700__ $$aChallinor, A
001596584 700__ $$aChamballu, A
001596584 700__ $$aChen, X
001596584 700__ $$aChiang, H C
001596584 700__ $$aChiang, L -Y
001596584 700__ $$aChristensen, P R
001596584 700__ $$aChurch, S
001596584 700__ $$aClements, D L
001596584 700__ $$aColombi, S
001596584 700__ $$aColombo, L P L
001596584 700__ $$aCouchot, F
001596584 700__ $$0AUTHOR|(CDS)2079675$$9#BEARD#$$aCoulais, A
001596584 700__ $$aCrill, B P
001596584 700__ $$aCurto, A
001596584 700__ $$aCuttaia, F
001596584 700__ $$aDanese, L
001596584 700__ $$aDavies, R D
001596584 700__ $$aDavis, R J
001596584 700__ $$ade Bernardis, P
001596584 700__ $$0AUTHOR|(CDS)2070255$$9#BEARD#$$ade Rosa, A
001596584 700__ $$ade Zotti, G
001596584 700__ $$aDelabrouille, J
001596584 700__ $$aDelouis, J -M
001596584 700__ $$aDésert, F -X
001596584 700__ $$aDickinson, C
001596584 700__ $$aDiego, J M
001596584 700__ $$aDole, H
001596584 700__ $$aDonzelli, S
001596584 700__ $$aDoré, O
001596584 700__ $$aDouspis, M
001596584 700__ $$aDupac, X
001596584 700__ $$aEfstathiou, G
001596584 700__ $$aEnßlin, T A
001596584 700__ $$aEriksen, H K
001596584 700__ $$aFinelli, F
001596584 700__ $$aForni, O
001596584 700__ $$aFrailis, M
001596584 700__ $$aFranceschi, E
001596584 700__ $$aGaleotta, S
001596584 700__ $$aGanga, K
001596584 700__ $$aGhosh, T
001596584 700__ $$aGiard, M
001596584 700__ $$aGiraud-Héraud, Y
001596584 700__ $$aGonzález-Nuevo, J
001596584 700__ $$aGórski, K M
001596584 700__ $$aGratton, S
001596584 700__ $$aGregorio, A
001596584 700__ $$aGruppuso, A
001596584 700__ $$aHansen, F K
001596584 700__ $$aHanson, D
001596584 700__ $$aHarrison, D
001596584 700__ $$aHelou, G
001596584 700__ $$aHenrot-Versillé, S
001596584 700__ $$aHernández-Monteagudo, C
001596584 700__ $$aHerranz, D
001596584 700__ $$aHildebrandt, S R
001596584 700__ $$aHivon, E
001596584 700__ $$aHobson, M
001596584 700__ $$aHolmes, W A
001596584 700__ $$aHornstrup, A
001596584 700__ $$aHovest, W
001596584 700__ $$aHuffenberger, K M
001596584 700__ $$aJaffe, A H
001596584 700__ $$aJaffe, T R
001596584 700__ $$aJones, W C
001596584 700__ $$aJuvela, M
001596584 700__ $$aKalberla, P
001596584 700__ $$aKeihänen, E
001596584 700__ $$aKerp, J
001596584 700__ $$aKeskitalo, R
001596584 700__ $$aKisner, T S
001596584 700__ $$aKneissl, R
001596584 700__ $$aKnoche, J
001596584 700__ $$aKnox, L
001596584 700__ $$aKunz, M
001596584 700__ $$aKurki-Suonio, H
001596584 700__ $$aLacasa, F
001596584 700__ $$aLagache, G
001596584 700__ $$aLähteenmäki, A
001596584 700__ $$aLamarre, J -M
001596584 700__ $$aLanger, M
001596584 700__ $$aLasenby, A
001596584 700__ $$aLaureijs, R J
001596584 700__ $$aLawrence, C R
001596584 700__ $$0AUTHOR|(CDS)2094138$$9#BEARD#$$aLeonardi, R
001596584 700__ $$aLeón-Tavares, J
001596584 700__ $$0AUTHOR|(CDS)2070506$$9#BEARD#$$aLesgourgues, J$$uLPHE, Lausanne$$uCERN
001596584 700__ $$aLiguori, M
001596584 700__ $$aLilje, P B
001596584 700__ $$aLinden-Vørnle, M
001596584 700__ $$aLópez-Caniego, M
001596584 700__ $$aLubin, P M
001596584 700__ $$aMacías-Pérez, J F
001596584 700__ $$aMaffei, B
001596584 700__ $$aMaino, D
001596584 700__ $$aMandolesi, N
001596584 700__ $$aMaris, M
001596584 700__ $$aMarshall, D J
001596584 700__ $$aMartin, P G
001596584 700__ $$aMartínez-González, E
001596584 700__ $$aMasi, S
001596584 700__ $$aMatarrese, S
001596584 700__ $$aMatthai, F
001596584 700__ $$aMazzotta, P
001596584 700__ $$aMelchiorri, A
001596584 700__ $$aMendes, L
001596584 700__ $$aMennella, A
001596584 700__ $$aMigliaccio, M
001596584 700__ $$0AUTHOR|(CDS)2084651$$9#BEARD#$$aMitra, S
001596584 700__ $$aMiville-Deschênes, M -A
001596584 700__ $$aMoneti, A
001596584 700__ $$aMontier, L
001596584 700__ $$aMorgante, G
001596584 700__ $$aMortlock, D
001596584 700__ $$aMunshi, D
001596584 700__ $$aMurphy, J A
001596584 700__ $$aNaselsky, P
001596584 700__ $$aNati, F
001596584 700__ $$aNatoli, P
001596584 700__ $$aNetterfield, C B
001596584 700__ $$aNørgaard-Nielsen, H U
001596584 700__ $$aNoviello, F
001596584 700__ $$aNovikov, D
001596584 700__ $$aNovikov, I
001596584 700__ $$aOsborne, S
001596584 700__ $$aOxborrow, C A
001596584 700__ $$aPaci, F
001596584 700__ $$aPagano, L
001596584 700__ $$aPajot, F
001596584 700__ $$aPaladini, R
001596584 700__ $$aPaoletti, D
001596584 700__ $$aPartridge, B
001596584 700__ $$aPasian, F
001596584 700__ $$aPatanchon, G
001596584 700__ $$aPerdereau, O
001596584 700__ $$aPerotto, L
001596584 700__ $$aPerrotta, F
001596584 700__ $$aPiacentini, F
001596584 700__ $$0AUTHOR|(CDS)2081174$$9#BEARD#$$aPiat, M
001596584 700__ $$aPierpaoli, E
001596584 700__ $$aPietrobon, D
001596584 700__ $$aPlaszczynski, S
001596584 700__ $$aPointecouteau, E
001596584 700__ $$aPolenta, G
001596584 700__ $$aPonthieu, N
001596584 700__ $$aPopa, L
001596584 700__ $$aPoutanen, T
001596584 700__ $$aPratt, G W
001596584 700__ $$aPrézeau, G
001596584 700__ $$aPrunet, S
001596584 700__ $$aPuget, J -L
001596584 700__ $$aRachen, J P
001596584 700__ $$aReach, W T
001596584 700__ $$aRebolo, R
001596584 700__ $$aReinecke, M
001596584 700__ $$aRemazeilles, M
001596584 700__ $$aRenault, C
001596584 700__ $$aRicciardi, S
001596584 700__ $$aRiller, T
001596584 700__ $$aRistorcelli, I
001596584 700__ $$aRocha, G
001596584 700__ $$aRosset, C
001596584 700__ $$aRoudier, G
001596584 700__ $$aRowan-Robinson, M
001596584 700__ $$aRubiño-Martín, J A
001596584 700__ $$aRusholme, B
001596584 700__ $$aSandri, M
001596584 700__ $$aSantos, D
001596584 700__ $$aSavini, G
001596584 700__ $$aScott, D
001596584 700__ $$aSeiffert, M D
001596584 700__ $$aSerra, P
001596584 700__ $$aShellard, E P S
001596584 700__ $$aSpencer, L D
001596584 700__ $$aStarck, J -L
001596584 700__ $$aStolyarov, V
001596584 700__ $$aStompor, R
001596584 700__ $$aSudiwala, R
001596584 700__ $$aSunyaev, R
001596584 700__ $$aSureau, F
001596584 700__ $$aSutton, D
001596584 700__ $$aSuur-Uski, A -S
001596584 700__ $$aSygnet, J -F
001596584 700__ $$aTauber, J A
001596584 700__ $$aTavagnacco, D
001596584 700__ $$aTerenzi, L
001596584 700__ $$aToffolatti, L
001596584 700__ $$aTomasi, M
001596584 700__ $$aTristram, M
001596584 700__ $$aTucci, M
001596584 700__ $$aTuovinen, J
001596584 700__ $$aTürler, M
001596584 700__ $$aValenziano, L
001596584 700__ $$aValiviita, J
001596584 700__ $$aVan Tent, B
001596584 700__ $$aVielva, P
001596584 700__ $$aVilla, F
001596584 700__ $$aVittorio, N
001596584 700__ $$aWade, L A
001596584 700__ $$aWandelt, B D
001596584 700__ $$aWelikala, N
001596584 700__ $$aWhite, M
001596584 700__ $$aWhite, S D M
001596584 700__ $$aWinkel, B
001596584 700__ $$aYvon, D
001596584 700__ $$aZacchei, A
001596584 700__ $$aZonca, A
001596584 710__ $$gPlanck Collaboration
001596584 773__ $$cA30$$pAstron. Astrophys.$$v571$$y2014
001596584 8564_ $$uhttp://arxiv.org/pdf/1309.0382.pdf$$yPreprint
001596584 8564_ $$uhttp://www.aanda.org/articles/aa/pdf/2014/11/aa22093-13.pdf$$yEDP Sciences Free Access article
001596584 916__ $$sn$$w201335$$ya2014
001596584 960__ $$a13
001596584 980__ $$aARTICLE