dc.contributor.author |
Ade P. |
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dc.contributor.author |
Aghanim N. |
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dc.contributor.author |
Arnaud M. |
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dc.contributor.author |
Ashdown M. |
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dc.contributor.author |
Aubourg E. |
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dc.contributor.author |
Aumont J. |
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dc.contributor.author |
Baccigalupi C. |
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dc.contributor.author |
Banday A. |
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dc.contributor.author |
Barreiro R. |
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dc.contributor.author |
Bartolo N. |
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dc.contributor.author |
Battaner E. |
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dc.contributor.author |
Benabed K. |
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dc.contributor.author |
Benoit-Lévy A. |
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dc.contributor.author |
Bersanelli M. |
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dc.contributor.author |
Bielewicz P. |
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dc.contributor.author |
Bock J. |
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dc.contributor.author |
Bonaldi A. |
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dc.contributor.author |
Bonavera L. |
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dc.contributor.author |
Bond J. |
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dc.contributor.author |
Borrill J. |
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dc.contributor.author |
Bouchet F. |
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dc.contributor.author |
Burigana C. |
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dc.contributor.author |
Calabrese E. |
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dc.contributor.author |
Cardoso J. |
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dc.contributor.author |
Catalano A. |
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dc.contributor.author |
Chamballu A. |
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dc.contributor.author |
Chiang H. |
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dc.contributor.author |
Christensen P. |
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dc.contributor.author |
Clements D. |
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dc.contributor.author |
Colombo L. |
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dc.contributor.author |
Combet C. |
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dc.contributor.author |
Crill B. |
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dc.contributor.author |
Curto A. |
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dc.contributor.author |
Cuttaia F. |
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dc.contributor.author |
Danese L. |
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dc.contributor.author |
Davies R. |
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dc.contributor.author |
Davis R. |
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dc.contributor.author |
De Bernardis P. |
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dc.contributor.author |
De Zotti G. |
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dc.contributor.author |
Delabrouille J. |
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dc.contributor.author |
Dickinson C. |
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dc.contributor.author |
Diego J. |
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dc.contributor.author |
Dolag K. |
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dc.contributor.author |
Donzelli S. |
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dc.contributor.author |
Doré O. |
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dc.contributor.author |
Douspis M. |
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dc.contributor.author |
Ducout A. |
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dc.contributor.author |
Dupac X. |
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dc.contributor.author |
Efstathiou G. |
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dc.contributor.author |
Elsner F. |
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dc.contributor.author |
Enßlin T. |
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dc.contributor.author |
Eriksen H. |
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dc.contributor.author |
Finelli F. |
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dc.contributor.author |
Forni O. |
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dc.contributor.author |
Frailis M. |
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dc.contributor.author |
Fraisse A. |
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dc.contributor.author |
Franceschi E. |
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dc.contributor.author |
Frejsel A. |
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dc.contributor.author |
Galeotta S. |
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dc.contributor.author |
Galli S. |
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dc.contributor.author |
Ganga K. |
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dc.contributor.author |
Génova-Santos R. |
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dc.contributor.author |
Giard M. |
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dc.contributor.author |
Gjerløw E. |
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dc.date.accessioned |
2018-09-19T20:04:51Z |
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dc.date.available |
2018-09-19T20:04:51Z |
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dc.date.issued |
2016 |
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dc.identifier.issn |
0004-6361 |
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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. |
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dc.relation.ispartofseries |
Astronomy and Astrophysics |
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dc.subject |
Cosmic background radiation |
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dc.subject |
Cosmology: observations |
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dc.subject |
Galaxies: clusters: intracluster medium |
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dc.subject |
Large-scale structure of Universe |
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dc.title |
Planck intermediate results: XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect |
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dc.type |
Article |
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dc.relation.ispartofseries-volume |
586 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.source.id |
SCOPUS00046361-2016-586-SID84958986338 |
|