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dc.contributor.author | Ade P. | |
dc.contributor.author | Aghanim N. | |
dc.contributor.author | Arnaud M. | |
dc.contributor.author | Ashdown M. | |
dc.contributor.author | Aubourg E. | |
dc.contributor.author | Aumont J. | |
dc.contributor.author | Baccigalupi C. | |
dc.contributor.author | Banday A. | |
dc.contributor.author | Barreiro R. | |
dc.contributor.author | Bartolo N. | |
dc.contributor.author | Battaner E. | |
dc.contributor.author | Benabed K. | |
dc.contributor.author | Benoit-Lévy A. | |
dc.contributor.author | Bersanelli M. | |
dc.contributor.author | Bielewicz P. | |
dc.contributor.author | Bock J. | |
dc.contributor.author | Bonaldi A. | |
dc.contributor.author | Bonavera L. | |
dc.contributor.author | Bond J. | |
dc.contributor.author | Borrill J. | |
dc.contributor.author | Bouchet F. | |
dc.contributor.author | Burigana C. | |
dc.contributor.author | Calabrese E. | |
dc.contributor.author | Cardoso J. | |
dc.contributor.author | Catalano A. | |
dc.contributor.author | Chamballu A. | |
dc.contributor.author | Chiang H. | |
dc.contributor.author | Christensen P. | |
dc.contributor.author | Clements D. | |
dc.contributor.author | Colombo L. | |
dc.contributor.author | Combet C. | |
dc.contributor.author | Crill B. | |
dc.contributor.author | Curto A. | |
dc.contributor.author | Cuttaia F. | |
dc.contributor.author | Danese L. | |
dc.contributor.author | Davies R. | |
dc.contributor.author | Davis R. | |
dc.contributor.author | De Bernardis P. | |
dc.contributor.author | De Zotti G. | |
dc.contributor.author | Delabrouille J. | |
dc.contributor.author | Dickinson C. | |
dc.contributor.author | Diego J. | |
dc.contributor.author | Dolag K. | |
dc.contributor.author | Donzelli S. | |
dc.contributor.author | Doré O. | |
dc.contributor.author | Douspis M. | |
dc.contributor.author | Ducout A. | |
dc.contributor.author | Dupac X. | |
dc.contributor.author | Efstathiou G. | |
dc.contributor.author | Elsner F. | |
dc.contributor.author | Enßlin T. | |
dc.contributor.author | Eriksen H. | |
dc.contributor.author | Finelli F. | |
dc.contributor.author | Forni O. | |
dc.contributor.author | Frailis M. | |
dc.contributor.author | Fraisse A. | |
dc.contributor.author | Franceschi E. | |
dc.contributor.author | Frejsel A. | |
dc.contributor.author | Galeotta S. | |
dc.contributor.author | Galli S. | |
dc.contributor.author | Ganga K. | |
dc.contributor.author | Génova-Santos R. | |
dc.contributor.author | Giard M. | |
dc.contributor.author | Gjerløw E. | |
dc.date.accessioned | 2018-09-19T20:04:51Z | |
dc.date.available | 2018-09-19T20:04:51Z | |
dc.date.issued | 2016 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/142522 | |
dc.description.abstract | © ESO, 2016.By looking at the kinetic Sunyaev-Zeldovich effect (kSZ) in Planck nominal mission data, we present a significant detection of baryons participating in large-scale bulk flows around central galaxies (CGs) at redshift z ≈ 0.1. We estimate the pairwise momentum of the kSZ temperature fluctuations at the positions of the Central Galaxy Catalogue (CGC) samples extracted from Sloan Digital Sky Survey (SDSS-DR7) data. For the foreground-cleaned SEVEM, SMICA, NILC, and COMMANDER maps, we find 1.8-2.5σ detections of the kSZ signal, which are consistent with the kSZ evidence found in individual Planck raw frequency maps, although lower than found in the WMAP-9yr W-band (3.3σ). We further reconstruct the peculiar velocity field from the CG density field, and compute for the first time the cross-correlation function between kSZ temperature fluctuations and estimates of CG radial peculiar velocities. This correlation function yields a 3.0-3.7σ detection of the peculiar motion of extended gas on Mpc scales in flows correlated up to distances of 80-100 h-1 Mpc. Both the pairwise momentum estimates and the kSZ temperature-velocity field correlation find evidence for kSZ signatures out to apertures of 8 arcmin and beyond, corresponding to a physical radius of >1 Mpc, more than twice the mean virial radius of halos. This is consistent with the predictions from hydrodynamical simulations that most of the baryons are outside the virialized halos. We fit a simple model, in which the temperature-velocity cross-correlation is proportional to the signal seen in a semi-analytic model built upon N-body simulations, and interpret the proportionality constant as an effective optical depth to Thomson scattering. We find τT = (1.4 ± 0.5) × 10-4; the simplest interpretation of this measurement is that much of the gas is in a diffuse phase, which contributes little signal to X-ray or thermal Sunyaev-Zeldovich observations. | |
dc.relation.ispartofseries | Astronomy and Astrophysics | |
dc.subject | Cosmic background radiation | |
dc.subject | Cosmology: observations | |
dc.subject | Galaxies: clusters: intracluster medium | |
dc.subject | Large-scale structure of Universe | |
dc.title | Planck intermediate results: XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect | |
dc.type | Article | |
dc.relation.ispartofseries-volume | 586 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS00046361-2016-586-SID84958986338 |