Planck 2015 results. XXI. The integrated Sachs-Wolfe effect
Journal
Date Issued
2016
Author(s)
Planck Collaboration
•
Ade, P. A. R.
•
Aghanim, N.
•
Arnaud, M.
•
Ashdown, M.
•
Aumont, J.
•
Baccigalupi, C.
•
Banday, A. J.
•
Barreiro, R. B.
•
Bartolo, N.
•
Basak, S.
•
•
de Zotti, G.
•
Delabrouille, J.
•
Désert, F. -X.
•
Diego, J. M.
•
Dole, H.
•
Donzelli, S.
•
Doré, O.
•
Douspis, M.
•
Knoche, J.
•
Prézeau, G.
•
Ducout, A.
•
Dupac, X.
•
Efstathiou, G.
•
Elsner, F.
•
Enßlin, T. A.
•
Eriksen, H. K.
•
Fergusson, J.
•
Fernandez-Cobos, R.
•
•
Forni, O.
•
Prunet, S.
•
Kunz, M.
•
•
Fraisse, A. A.
•
•
Frejsel, A.
•
•
Galli, S.
•
Ganga, K.
•
Génova-Santos, R. T.
•
Giard, M.
•
Puget, J. -L.
•
Giraud-Héraud, Y.
•
Battaner, E.
•
Gjerløw, E.
•
González-Nuevo, J.
•
Górski, K. M.
•
Gratton, S.
•
Gregorio, A.
•
•
Gudmundsson, J. E.
•
Hansen, F. K.
•
Rachen, J. P.
•
Hanson, D.
•
Harrison, D. L.
•
Kurki-Suonio, H.
•
Henrot-Versillé, S.
•
Hernández-Monteagudo, C.
•
Herranz, D.
•
Hildebrandt, S. R.
•
Hivon, E.
•
Hobson, M.
•
Holmes, W. A.
•
Reach, W. T.
•
Hornstrup, A.
•
Hovest, W.
•
Huffenberger, K. M.
•
Lagache, G.
•
Hurier, G.
•
Ilić, S.
•
Lähteenmäki, A.
•
Lamarre, J. -M.
•
Langer, M.
•
Lasenby, A.
•
Rebolo, R.
•
Lattanzi, M.
•
Lawrence, C. R.
•
Leonardi, R.
•
Lesgourgues, J.
•
Benabed, K.
•
Levrier, F.
•
Liguori, M.
•
Lilje, P. B.
•
Linden-Vørnle, M.
•
López-Caniego, M.
•
Reinecke, M.
•
Lubin, P. M.
•
Ma, Y. -Z.
•
Macías-Pérez, J. F.
•
•
Maino, D.
•
Benoît, A.
•
Mandolesi, N.
•
Mangilli, A.
•
Marcos-Caballero, A.
•
•
Remazeilles, M.
•
Martin, P. G.
•
Martínez-González, E.
•
Masi, S.
•
Matarrese, S.
•
McGehee, P.
•
Meinhold, P. R.
•
Benoit-Lévy, A.
•
Melchiorri, A.
•
Mendes, L.
•
Mennella, A.
•
Renault, C.
•
Migliaccio, M.
•
Mitra, S.
•
Miville-Deschênes, M. -A.
•
Moneti, A.
•
Montier, L.
•
•
Mortlock, D.
•
Bernard, J. -P.
•
Moss, A.
•
Munshi, D.
•
Bonaldi, A.
•
Murphy, J. A.
•
Naselsky, P.
•
Nati, F.
•
Natoli, P.
•
Netterfield, C. B.
•
Nørgaard-Nielsen, H. U.
•
Noviello, F.
•
Novikov, D.
•
Bersanelli, M.
•
Novikov, I.
•
Jaffe, A. H.
•
Oxborrow, C. A.
•
Paci, F.
•
Pagano, L.
•
Pajot, F.
•
•
Pasian, F.
•
Patanchon, G.
•
Perdereau, O.
•
Perotto, L.
•
Bielewicz, P.
•
Renzi, A.
•
Perrotta, F.
•
Pettorino, V.
•
Piacentini, F.
•
Piat, M.
•
Pierpaoli, E.
•
Pietrobon, D.
•
Plaszczynski, S.
•
Pointecouteau, E.
•
Polenta, G.
•
Popa, L.
•
Ristorcelli, I.
•
Bock, J. J.
•
Pratt, G. W.
•
Rocha, G.
•
Rosset, C.
•
•
Roudier, G.
•
Rubiño-Martín, J. A.
•
Rusholme, B.
•
•
Santos, D.
•
Jaffe, T. R.
•
Bonavera, L.
•
Savelainen, M.
•
Savini, G.
•
Schaefer, B. M.
•
Scott, D.
•
Seiffert, M. D.
•
Shellard, E. P. S.
•
Spencer, L. D.
•
Stolyarov, V.
•
Stompor, R.
•
Jones, W. C.
•
Sudiwala, R.
•
Bond, J. R.
•
Sunyaev, R.
•
Sutton, D.
•
Suur-Uski, A. -S.
•
Sygnet, J. -F.
•
Tauber, J. A.
•
•
Toffolatti, L.
•
Tomasi, M.
•
Juvela, M.
•
Tristram, M.
•
Tucci, M.
•
Borrill, J.
•
Tuovinen, J.
•
•
Valiviita, J.
•
Van Tent, F.
•
Vielva, P.
•
•
Wade, L. A.
•
Keihänen, E.
•
Wandelt, B. D.
•
Wehus, I. K.
•
Yvon, D.
•
Bouchet, F. R.
•
•
Zonca, A.
•
Bucher, M.
•
•
Butler, R. C.
•
Calabrese, E.
•
Keskitalo, R.
•
Cardoso, J. -F.
•
Casaponsa, B.
•
Catalano, A.
•
Challinor, A.
•
Chamballu, A.
•
Chiang, H. C.
•
Christensen, P. R.
•
Church, S.
•
Clements, D. L.
•
Colombi, S.
•
Kisner, T. S.
•
Colombo, L. P. L.
•
Combet, C.
•
Couchot, F.
•
Coulais, A.
•
Crill, B. P.
•
Curto, A.
•
•
Danese, L.
•
Davies, R. D.
•
Davis, R. J.
•
Kneissl, R.
•
de Bernardis, P.
Abstract
This paper presents a study of the integrated Sachs-Wolfe (ISW) effect from the Planck 2015 temperature and polarization data release. This secondary cosmic microwave background (CMB) anisotropy caused by the large-scale time-evolving gravitational potential is probed from different perspectives. The CMB is cross-correlated with different large-scale structure (LSS) tracers: radio sources from the NVSS catalogue; galaxies from the optical SDSS and the infrared WISE surveys; and the Planck 2015 convergence lensing map. The joint cross-correlation of the CMB with the tracers yields a detection at 4σ where most of the signal-to-noise is due to the Planck lensing and the NVSS radio catalogue. In fact, the ISW effect is detected from the Planck data only at ≈3σ (through the ISW-lensing bispectrum), which is similar to the detection level achieved by combining the cross-correlation signal coming from all the galaxy catalogues mentioned above. We study the ability of the ISW effect to place constraints on the dark-energy parameters; in particular, we show that ΩΛ is detected at more than 3σ. This cross-correlation analysis is performed only with the Planck temperature data, since the polarization scales available in the 2015 release do not permit significant improvement of the CMB-LSS cross-correlation detectability. Nevertheless, the Planck polarization data are used to study the anomalously large ISW signal previously reported through the aperture photometry on stacked CMB features at the locations of known superclusters and supervoids, which is in conflict with ΛCDM expectations. We find that the current Planck polarization data do not exclude that this signal could be caused by the ISW effect. In addition, the stacking of the Planck lensing map on the locations of superstructures exhibits a positive cross-correlation with these large-scale structures. Finally, we have improved our previous reconstruction of the ISW temperature fluctuations by combining the information encoded in all the previously mentioned LSS tracers. In particular, we construct a map of the ISW secondary anisotropies and the corresponding uncertainties map, obtained from simulations. We also explore the reconstruction of the ISW anisotropies caused by the large-scale structure traced by the 2MASS Photometric Redshift Survey (2MPZ) by directly inverting the density field into the gravitational potential field.
Volume
594
Start page
A21
Issn Identifier
0004-6361
Ads BibCode
2016A&A...594A..21P
Rights
open.access
File(s)![Thumbnail Image]()
![Thumbnail Image]()
Loading...
Name
1502.01595.pdf
Description
preprint
Size
26.55 MB
Format
Adobe PDF
Checksum (MD5)
407a58faed9d906e3fd35e82ba45ab36
Loading...
Name
aa25831-15_compressed.pdf
Description
pdf editoriale
Size
6.93 MB
Format
Adobe PDF
Checksum (MD5)
6a992b24c1b57adcb79e98fb002dacb9