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@article{Ade:2014:0004-6361/201321522,
author = {Ade, PAR and Aghanim, N and Armitage-Caplan, C and Arnaud, M and Ashdown, M and Atrio-Barandela, F and Aumont, J and Baccigalupi, C and Banday, AJ and Barreiro, B and Bartlett, JG and Battanerioo, E and Benabed, K and Benoit, A and Benoit-Levy, A and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bobin, J and Bock, JJ and Bonaldi, A and Bond, JR and Borrill, J and Bouchet, FR and Bridges, M and Bucher, M and Burigana, C and Butler, RC and Cardoso, J-F and Carvalho, P and Catalano, A and Challinor, A and Chamballu, A and Chiang, HC and Chiang, L-Y and Christensen, PR and Church, S and Clements, DL and Colombi, S and Colombo, LPL and Comis, B and Couchot, F and Coulais, A and Crill, BP and Curto, A and Cuttaia, F and Da, Silva A and Danese, L and Davies, RD and Davis, RJ and de, Bernardis P and de, Rosa A and de, Zotti G and Delabrouille, J and Delouis, J-M and Desert, F-X and Dickinson, C and Diego, JM and Dolag, K and Dole, H and Donzelli, S and Dore, A and Douspis, M and Dupac, X},
doi = {0004-6361/201321522},
journal = {ASTRONOMY & ASTROPHYSICS},
title = {Planck 2013 results. XXI. Power spectrum and high-order statistics of the Planck all-sky Compton parameter map},
url = {http://dx.doi.org/10.1051/0004-6361/201321522},
volume = {571},
year = {2014}
}

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TY  - JOUR
AB  - We have constructed the first all-sky map of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 100 to 857 GHz frequency channel maps from the Planck survey. This map shows an obvious galaxy cluster tSZ signal that is well matched with blindly detected clusters in the Planck SZ catalogue. To characterize the signal in the tSZ map we have computed its angular power spectrum. At large angular scales ( < 60), the major foreground contaminant is the diffuse thermal dust emission. At small angular scales ( > 500) the clustered cosmic infrared background and residual point sources are the major contaminants. These foregrounds are carefully modelled and subtracted. We thus measure the tSZ power spectrum over angular scales 0.17°  θ  3.0° that were previously unexplored. The measured tSZ power spectrum is consistent with that expected from the Planck catalogue of SZ sources, with clear evidence of additional signal from unresolved clusters and, potentially, diffuse warm baryons. Marginalized band-powers of the Planck tSZ power spectrum and the best-fit model are given. The non-Gaussianity of the Compton parameter map is further characterized by computing its 1D probability distribution function and its bispectrum. The measured tSZ power spectrum and high order statistics are used to place constraints on σ8.
AU  - Ade,PAR
AU  - Aghanim,N
AU  - Armitage-Caplan,C
AU  - Arnaud,M
AU  - Ashdown,M
AU  - Atrio-Barandela,F
AU  - Aumont,J
AU  - Baccigalupi,C
AU  - Banday,AJ
AU  - Barreiro,B
AU  - Bartlett,JG
AU  - Battanerioo,E
AU  - Benabed,K
AU  - Benoit,A
AU  - Benoit-Levy,A
AU  - Bernard,J-P
AU  - Bersanelli,M
AU  - Bielewicz,P
AU  - Bobin,J
AU  - Bock,JJ
AU  - Bonaldi,A
AU  - Bond,JR
AU  - Borrill,J
AU  - Bouchet,FR
AU  - Bridges,M
AU  - Bucher,M
AU  - Burigana,C
AU  - Butler,RC
AU  - Cardoso,J-F
AU  - Carvalho,P
AU  - Catalano,A
AU  - Challinor,A
AU  - Chamballu,A
AU  - Chiang,HC
AU  - Chiang,L-Y
AU  - Christensen,PR
AU  - Church,S
AU  - Clements,DL
AU  - Colombi,S
AU  - Colombo,LPL
AU  - Comis,B
AU  - Couchot,F
AU  - Coulais,A
AU  - Crill,BP
AU  - Curto,A
AU  - Cuttaia,F
AU  - Da,Silva A
AU  - Danese,L
AU  - Davies,RD
AU  - Davis,RJ
AU  - de,Bernardis P
AU  - de,Rosa A
AU  - de,Zotti G
AU  - Delabrouille,J
AU  - Delouis,J-M
AU  - Desert,F-X
AU  - Dickinson,C
AU  - Diego,JM
AU  - Dolag,K
AU  - Dole,H
AU  - Donzelli,S
AU  - Dore,A
AU  - Douspis,M
AU  - Dupac,X
AU  - Efstathiou,G
AU  - Ensslin,TA
AU  - Eriksen,HK
AU  - Finelli,F
AU  - Flores-Cacho,I
AU  - Forni,O
AU  - Frailis,M
AU  - Franceschi,E
AU  - Galeotta,S
AU  - Ganga,K
AU  - Genova-Santos,RT
AU  - Giard,M
AU  - Giardino,G
AU  - Giraud-Heraud,Y
AU  - Gonzalez-Nuevo,J
AU  - Gorski,KM
AU  - Gratton,S
AU  - Gregorio,A
AU  - Gruppuso,A
AU  - Hansen,FK
AU  - Hanson,D
AU  - Harrison,D
AU  - Henrot-Versille,S
AU  - Hernandez-Monteagudo,C
AU  - Herranz,D
AU  - Hildebrandt,SR
AU  - Hivon,E
AU  - Hobson,M
AU  - Holmes,WA
AU  - Hornstrup,A
AU  - Hovest,W
AU  - Huffenberger,KM
AU  - Hurier,G
AU  - Jaffe,AH
AU  - Jaffe,TR
AU  - Jones,WC
AU  - Juvela,M
AU  - Keihanen,E
AU  - Keskitalo,R
AU  - Kisner,TS
AU  - Kneissl,R
AU  - Knoche,J
AU  - Knox,L
AU  - Kunz,M
AU  - Kurki-Suonio,H
AU  - Lacasa,F
AU  - Lagache,G
AU  - Lahteenmaki,A
AU  - Lamarre,J-M
AU  - Lasenby,A
AU  - Laureijs,RJ
AU  - Lawrence,CR
AU  - Leahy,JP
AU  - Leonardi,R
AU  - Loen-Tavares,J
AU  - Lesgourgues,J
AU  - Liguori,M
AU  - Lilje,PB
AU  - Linden-Vornle,M
AU  - Lopez-Caniego,M
AU  - Lubin,PM
AU  - Macias-Perez,JF
AU  - Maffei,B
AU  - Maino,D
AU  - Mandolesi,N
AU  - Marcos-Caballero,A
AU  - Maris,M
AU  - Marshall,DJ
AU  - Martin,G
AU  - Macinez-Gonzalez,E
AU  - Masi,S
AU  - Massardi,M
AU  - Matarrese,S
AU  - Matthai,F
AU  - Mazzotta,P
AU  - Melchiorri,A
AU  - Melin,J-B
AU  - Mendes,L
AU  - Mennella,A
AU  - Migliaccio,M
AU  - Mitra,S
AU  - Miville-Deschenes,M-A
AU  - Moneti,A
AU  - Montier,L
AU  - Morgante,G
AU  - Mortlock,D
AU  - Moss,A
AU  - Munshi,D
AU  - Naselsky,P
AU  - Nati,F
AU  - Natoli,P
AU  - Netterfield,CB
AU  - Norgaard-Nielsen,HU
AU  - Noviello,F
AU  - Novikov,D
AU  - Novikov,I
AU  - Osborne,S
AU  - Oxborrow,CA
AU  - Paci,F
AU  - Pagano,L
AU  - Pajot,F
AU  - Paoletti,D
DO  - 0004-6361/201321522
PY  - 2014///
SN  - 1432-0746
TI  - Planck 2013 results. XXI. Power spectrum and high-order statistics of the Planck all-sky Compton parameter map
T2  - ASTRONOMY & ASTROPHYSICS
UR  - http://dx.doi.org/10.1051/0004-6361/201321522
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000345282600002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - http://hdl.handle.net/10044/1/60725
VL  - 571
ER  -

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