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  5. Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect
 

Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2016
Author(s)
Planck Collaboration
•
Aghanim, N.
•
Arnaud, M.
•
Ashdown, M.
•
Aumont, J.
•
Baccigalupi, C.
•
Banday, A. J.
•
Barreiro, R. B.
•
Bartlett, J. G.
•
Bartolo, N.
•
Battaner, E.
•
Hansen, F. K.
•
Harrison, D. L.
•
Henrot-Versillé, S.
•
Hernández-Monteagudo, C.
•
Herranz, D.
•
Hildebrandt, S. R.
•
Hivon, E.
•
Holmes, W. A.
•
Hornstrup, A.
•
Liguori, M.
•
Suur-Uski, A. -S.
•
Huffenberger, K. M.
•
Hurier, G.
•
Jaffe, A. H.
•
Jones, W. C.
•
Juvela, M.
•
Keihänen, E.
•
Keskitalo, R.
•
Kneissl, R.
•
Knoche, J.
•
Kunz, M.
•
Sygnet, J. -F.
•
Lilje, P. B.
•
Kurki-Suonio, H.
•
Lacasa, F.
•
Battye, R.
•
Linden-Vørnle, M.
•
López-Caniego, M.
•
Macías-Pérez, J. F.
•
Maffei, B.
•
Maggio, G.  
•
Maino, D.
•
Tauber, J. A.
•
Mandolesi, N.
•
Mangilli, A.
•
Maris, M.  
•
Martin, P. G.
•
Benabed, K.
•
Martínez-González, E.
•
Masi, S.
•
Matarrese, S.
•
Melchiorri, A.
•
Melin, J. -B.
•
TERENZI, LUCA  
•
Migliaccio, M.
•
Miville-Deschênes, M. -A.
•
Moneti, A.
•
Montier, L.
•
MORGANTE, GIANLUCA  
•
Benoît, A.
•
Mortlock, D.
•
Munshi, D.
•
Murphy, J. A.
•
Naselsky, P.
•
Toffolatti, L.
•
Nati, F.
•
Natoli, P.
•
Noviello, F.
•
Novikov, D.
•
Novikov, I.
•
Paci, F.
•
Benoit-Lévy, A.
•
Pagano, L.
•
Pajot, F.
•
PAOLETTI, DANIELA  
•
Tomasi, M.
•
Pasian, F.
•
Patanchon, G.
•
Perdereau, O.
•
Perotto, L.
•
Pettorino, V.
•
Piacentini, F.
•
Piat, M.
•
Bernard, J. -P.
•
Pierpaoli, E.
•
Pietrobon, D.
•
Tramonte, D.
•
Plaszczynski, S.
•
Pointecouteau, E.
•
Polenta, G.
•
Ponthieu, N.
•
Pratt, G. W.
•
Prunet, S.
•
Puget, J. -L.
•
Rachen, J. P.
•
Bersanelli, M.
•
Reinecke, M.
•
Tristram, M.
•
Remazeilles, M.
•
Renault, C.
•
Renzi, A.
•
Ristorcelli, I.
•
Rocha, G.
•
ROSSETTI, MARIACHIARA  
•
Roudier, G.
•
Rubiño-Martín, J. A.
•
Rusholme, B.
•
Bielewicz, P.
•
Tucci, M.
•
SANDRI, MAURA  
•
Santos, D.
•
Sauvé, A.
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Savelainen, M.
•
Savini, G.
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Scott, D.
•
Spencer, L. D.
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Stolyarov, V.
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Stompor, R.
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Sunyaev, R.
•
Bonaldi, A.
•
Bock, J. J.
•
Sutton, D.
•
Lagache, G.
•
Tuovinen, J.
•
VALENZIANO, LUCA  
•
Valiviita, J.
•
Van Tent, B.
•
Vielva, P.
•
VILLA, FABRIZIO  
•
Wade, L. A.
•
Wandelt, B. D.
•
Wehus, I. K.
•
Yvon, D.
•
Lähteenmäki, A.
•
Bonavera, L.
•
ZACCHEI, Andrea  
•
Zonca, A.
•
Bond, J. R.
•
Borrill, J.
•
Bouchet, F. R.
•
BURIGANA, CARLO  
•
Butler, R. C.
•
Calabrese, E.
•
Cardoso, J. -F.
•
Lamarre, J. -M.
•
Catalano, A.
•
Challinor, A.
•
Chiang, H. C.
•
Christensen, P. R.
•
Churazov, E.
•
Clements, D. L.
•
Colombo, L. P. L.
•
Combet, C.
•
Comis, B.
•
Coulais, A.
•
Lasenby, A.
•
Crill, B. P.
•
Curto, A.
•
CUTTAIA, FRANCESCO  
•
Danese, L.
•
Davies, R. D.
•
Davis, R. J.
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de Bernardis, P.
•
De Rosa, A.  
•
de Zotti, G.
•
Delabrouille, J.
•
Lattanzi, M.
•
Désert, F. -X.
•
Dickinson, C.
•
Diego, J. M.
•
Dolag, K.
•
Dole, H.
•
Donzelli, S.
•
Doré, O.
•
Douspis, M.
•
Ducout, A.
•
Dupac, X.
•
Leonardi, R.
•
Efstathiou, G.
•
Elsner, F.
•
Enßlin, T. A.
•
Eriksen, H. K.
•
Fergusson, J.
•
FINELLI, FABIO  
•
Forni, O.
•
FRAILIS, Marco  
•
Fraisse, A. A.
•
FRANCESCHI, ENRICO  
•
Lesgourgues, J.
•
Frejsel, A.
•
GALEOTTA, Samuele  
•
Galli, S.
•
Ganga, K.
•
Génova-Santos, R. T.
•
Giard, M.
•
González-Nuevo, J.
•
Górski, K. M.
•
Gregorio, A.
•
GRUPPUSO, ALESSANDRO  
•
Levrier, F.
•
Gudmundsson, J. E.
DOI
10.1051/0004-6361/201525826
Abstract
We have constructed all-sky Compton parameters maps, y-maps, of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency channel maps from the Planck satellite. These reconstructed y-maps are delivered as part of the Planck 2015 release. The y-maps are characterized in terms of noise properties and residual foreground contamination, mainly thermal dust emission at large angular scales, and cosmic infrared background and extragalactic point sources at small angular scales. Specific masks are defined to minimize foreground residuals and systematics. Using these masks, we compute the y-map angular power spectrum and higher order statistics. From these we conclude that the y-map is dominated by tSZ signal in the multipole range, 20 <ℓ< 600. We compare the measured tSZ power spectrum and higher order statistics to various physically motivated models and discuss the implications of our results in terms of cluster physics and cosmology.
Volume
594
Start page
A22
Uri
http://hdl.handle.net/20.500.12386/25254
Url
https://www.aanda.org/articles/aa/abs/2016/10/aa25826-15/aa25826-15.html
Issn Identifier
0004-6361
Ads BibCode
2016A&A...594A..22P
Rights
open.access
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