Planck intermediate results LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect
| العنوان: | Planck intermediate results LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect |
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| المؤلفون: | Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Battye, R., Benabed, K., Bernard, J. -P, Bersanelli, M., Bielewicz, P., Bond, J. R., Borrill, J., Bouchet, F. R., Burigana, C., Calabrese, E., Carron, J., Chiang, H. C., Comis, B., Contreras, D., Crill, B. P., Curto, A., Cuttaia, F., Bernardis, P., Rosa, A., Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J. M., Doré, O., Ducout, A., Dupac, X., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Fantaye, Y., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A. A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Gerbino, M., Górski, K. M., Gruppuso, A., Gudmundsson, J. E., Handley, W., Hansen, F. K., Herranz, D., Eric Hivon, Huang, Z., Jaffe, A. H., Keihänen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lamarre, J. -M, Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Levrier, F., Liguori, M., Lilje, P. B., Lindholm, V., López-Caniego, M., Lubin, P. M., Ma, Y. -Z, Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Martin, P. G., Martínez-González, E., Matarrese, S., Mauri, N., Mcewen, J. D., Melchiorri, A., Mennella, A., Migliaccio, M., Miville-Deschênes, M. -A, Molinari, D., Moneti, A., Montier, L., Morgante, G., Natoli, P., Oxborrow, C. A., Pagano, L., Paoletti, D., Partridge, B., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Plaszczynski, S., Polastri, L., Polenta, G., Rachen, J. P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Roudier, G., Ruiz-Granados, B., Sandri, M., Savelainen, M., Scott, D., Sirignano, C., Sirri, G., Spencer, L. D., Stanco, L., Sunyaev, R., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Tent, F., Vielva, P., Villa, F., Vittorio, N., Wandelt, B. D., Wehus, I. K., Zacchei, A., Zonca, A. |
| المساهمون: | Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), APC - Gravitation (APC-Gravitation), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Battye, R., Benabed, K., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bond, J. R., Borrill, J., Bouchet, F. R., Burigana, C., Calabrese, E., Carron, J., Chiang, H.C., Comis, B., Contreras, D., Crill, B. P., Curto, A., Cuttaia, F., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J. M., Doré, O., Ducout, A., Dupac, X., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Fantaye, Y., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A. A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Gerbino, M., Górski, K. M., Gruppuso, A., Gudmundsson, J. E., Handley, W., Hansen, F. K., Herranz, D., Hivon, E., Huang, Z., Jaffe, A. H., Keihänen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lamarre, J.-M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Levrier, F., Liguori, M., Lilje, P. B., Lindholm, V., López-Caniego, M., Lubin, P. M., Ma, Y.-Z., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Martin, P. G., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J. D., Melchiorri, A., Mennella, A., Migliaccio, M., Miville-Deschênes, M.-A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Natoli, P., Oxborrow, C. A., Pagano, L., Paoletti, D., Partridge, B., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Plaszczynski, S., Polastri, L., Polenta, G., Rachen, J. P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Roudier, G., Ruiz-Granados, B., Sandri, M., Savelainen, M., Scott, D., Sirignano, C., Sirri, G., Spencer, L. D., Stanco, L., Sunyaev, R., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Van Tent, F., Vielva, P., Villa, F., Vittorio, N., Wandelt, B. D., Wehus, I. K., Zacchei, A., Zonca, A., Department of Physics, Helsinki Institute of Physics |
| المصدر: | Astronomy & Astrophysics, 617, pp. 1-17 NASA Astrophysics Data System Aghanim, N, Akrami, Y, Ashdown, M, Aumont, J, Baccigalupi, C, Ballardini, M, Banday, A J, Barreiro, R B, Bartolo, N, Basak, S, Battye, R, Benabed, K, Bernard, J P, Bersanelli, M, Bielewicz, P, Bond, J R, Borrill, J, Bouchet, F R, Burigana, C, Calabrese, E, Carron, J, Chiang, H C, Comis, B, Contreras, D, Crill, B P, Curto, A, Cuttaia, F, De Bernardis, P, De Rosa, A, De Zotti, G, Delabrouille, J, Di Valentino, E, Dickinson, C, Diego, J M, Doré, O, Ducout, A, Dupac, X, Elsner, F, Enßlin, T A, Eriksen, H K, Falgarone, E, Fantaye, Y, Finelli, F, Forastieri, F, Fraisse, A A, Hansen, F K, Kim, J, Ma, Y Z, Martin, P G, Oxborrow, C A, Pagano, L, Paoletti, D, Partridge, B, Perdereau, O, Perotto, L, Pettorino, V, Piacentini, F, Plaszczynski, S, Polastri, L, Polenta, G, Rachen, J P, Racine, B, Reinecke, M, Remazeilles, M, Renzi, A, Rocha, G, Roudier, G, Ruiz-Granados, B, Sandri, M, Savelainen, M, Scott, D, Sirignano, C, Sirri, G, Spencer, L D, Stanco, L, Sunyaev, R, Tauber, J A, Tavagnacco, D, Tenti, M, Toffolatti, L, Tomasi, M, Tristram, M, Trombetti, T, Valiviita, J, Van Tent, F, Vielva, P, Villa, F, Vittorio, N, Wandelt, B D, Wehus, I K, Zacchei, A & Zonca, A 2018, ' Planck intermediate results: LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect ', Astronomy and Astrophysics, vol. 617, A48 . https://doi.org/10.1051/0004-6361/201731489 Astronomy and Astrophysics-A&A Astronomy and Astrophysics-A&A, 2018, 617, pp.A48. ⟨10.1051/0004-6361/201731489⟩ Astronomy & Astrophysics, 617, 1-17 Astronomy & Astrophysics, 617, A48 Collaboration, P, Aghanim, N, Akrami, Y, Ashdown, M, Aumont, J, Baccigalupi, C, Ballardini, M, Banday, A J, Barreiro, R B, Bartolo, N, Basak, S, Battye, R, Benabed, K, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bond, J R, Borrill, J, Bouchet, F R, Burigana, C, Calabrese, E, Carron, J, Chiang, H C, Comis, B, Contreras, D, Crill, B P, Curto, A, Cuttaia, F, Bernardis, P D, Rosa, A D, Zotti, G D, Delabrouille, J, Valentino, E D, Dickinson, C, Diego, J M, Doré, O, Ducout, A, Dupac, X, Elsner, F, Enßlin, T A, Eriksen, H K, Falgarone, E, Fantaye, Y, Finelli, F, Forastieri, F, Frailis, M, Fraisse, A A, Franceschi, E, Frolov, A, Galeotta, S, Galli, S, Ganga, K, Gerbino, M, Górski, K M, Gruppuso, A, Gudmundsson, J E, Handley, W, Hansen, F K, Herranz, D, Hivon, E, Huang, Z, Jaffe, A H, Keihänen, E, Keskitalo, R, Kiiveri, K, Kim, J, Kisner, T S, Krachmalnicoff, N, Kunz, M, Kurki-Suonio, H, Lamarre, J-M, Lasenby, A, Lattanzi, M, Lawrence, C R, Jeune, M L, Levrier, F, Liguori, M, Lilje, P B, Lindholm, V, López-Caniego, M, Lubin, P M, Ma, Y-Z, Macías-Pérez, J F, Maggio, G, Maino, D, Mandolesi, N, Mangilli, A, Martin, P G, Martínez-González, E, Matarrese, S, Mauri, N, McEwen, J D, Melchiorri, A, Mennella, A, Migliaccio, M, Miville-Deschênes, M-A, Molinari, D, Moneti, A, Montier, L, Morgante, G, Natoli, P, Oxborrow, C A, Pagano, L, Paoletti, D, Partridge, B, Perdereau, O, Perotto, L, Pettorino, V, Piacentini, F, Plaszczynski, S, Polastri, L, Polenta, G, Rachen, J P, Racine, B, Reinecke, M, Remazeilles, M, Renzi, A, Rocha, G, Roudier, G, Ruiz-Granados, B, Sandri, M, Savelainen, M, Scott, D, Sirignano, C, Sirri, G, Spencer, L D, Stanco, L, Sunyaev, R, Tauber, J A, Tavagnacco, D, Tenti, M, Toffolatti, L, Tomasi, M, Tristram, M, Trombetti, T, Valiviita, J, Tent, F V, Vielva, P, Villa, F, Vittorio, N, Wandelt, B D, Wehus, I K, Zacchei, A & Zonca, A 2018, ' Planck intermediate results. LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect ', Astronomy and Astrophysics, vol. 617 . https://doi.org/10.1051/0004-6361/201731489 |
| سنة النشر: | 2018 |
| مصطلحات موضوعية: | Cosmology and Nongalactic Astrophysics (astro-ph.CO), Large-scale structure of Universe, Astronomy, Cosmic microwave background, FOS: Physical sciences, GALAXY CLUSTER SURVEY, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, clusters: general [Galaxies], Kinetic energy, Cosmic background radiation, H(-1) MPC SCALES, 114 Physical sciences, 01 natural sciences, NO, symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, ELLIPTIC GALAXIES, Methods: data analysis, 0103 physical sciences, Dispersion (optics), Optical depth (astrophysics), Planck, data analysis [Methods], 010303 astronomy & astrophysics, Physics, cosmic background radiation / large-scale structure of Universe / galaxies: clusters: general / methods: data analysis, 010308 nuclear & particles physics, cosmicbackgroundradiation–large-scalestructureofUniverse–galaxies:clusters:general–methods:dataanalysis, Velocity dispersion, Order (ring theory), BULK FLOWS, Astronomy and Astrophysics, Galaxies: clusters: general, Space and Planetary Science, DISTANT CLUSTERS, 115 Astronomy, Space science, Galaxy, MICROWAVE BACKGROUND MAPS, INTERNAL LINEAR COMBINATION, SCALE PECULIAR VELOCITIES, X-RAY, COSMIC FLOWS, astro-ph.CO, symbols, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics |
| الوصف: | Using the ${\it Planck}$ full-mission data, we present a detection of the temperature (and therefore velocity) dispersion due to the kinetic Sunyaev-Zeldovich (kSZ) effect from clusters of galaxies. To suppress the primary CMB and instrumental noise we derive a matched filter and then convolve it with the ${\it Planck}$ foreground-cleaned `${\tt 2D-ILC\,}$' maps. By using the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we determine the normalized ${\it rms}$ dispersion of the temperature fluctuations at the positions of clusters, finding that this shows excess variance compared with the noise expectation. We then build an unbiased statistical estimator of the signal, determining that the normalized mean temperature dispersion of $1526$ clusters is $\langle \left(\Delta T/T \right)^{2} \rangle = (1.64 \pm 0.48) \times 10^{-11}$. However, comparison with analytic calculations and simulations suggest that around $0.7\,\sigma$ of this result is due to cluster lensing rather than the kSZ effect. By correcting this, the temperature dispersion is measured to be $\langle \left(\Delta T/T \right)^{2} \rangle = (1.35 \pm 0.48) \times 10^{-11}$, which gives a detection at the $2.8\,\sigma$ level. We further convert uniform-weight temperature dispersion into a measurement of the line-of-sight velocity dispersion, by using estimates of the optical depth of each cluster (which introduces additional uncertainty into the estimate). We find that the velocity dispersion is $\langle v^{2} \rangle =(123\,000 \pm 71\,000)\,({\rm km}\,{\rm s}^{-1})^{2}$, which is consistent with findings from other large-scale structure studies, and provides direct evidence of statistical homogeneity on scales of $600\,h^{-1}{\rm Mpc}$. Our study shows the promise of using cross-correlations of the kSZ effect with large-scale structure in order to constrain the growth of structure. Comment: 20 pages, 12 figures and 8 tables, A&A in press |
| وصف الملف: | application/pdf; STAMPA |
| تدمد: | 0004-6361 1432-0746 |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdd3d22dd78dce9665c8295138f9a2e3 https://doi.org/10.1051/0004-6361/201731489 |
| حقوق: | OPEN |
| رقم الأكسشن: | edsair.doi.dedup.....fdd3d22dd78dce9665c8295138f9a2e3 |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 00046361 14320746 |
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