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Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts - CERN Document Server
<!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.0 Transitional//EN" "http://www.w3.org/TR/xhtml1/DTD/xhtml1-transitional.dtd"> <!--[if IEMobile 7]><html class="iem7" xmlns="http://www.w3.org/1999/xhtml" lang="ru" xml:lang="ru" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if lte IE 6]><html class="ie6 ie6-7 ie6-8" xmlns="http://www.w3.org/1999/xhtml" lang="ru" xml:lang="ru" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if (IE 7)&(!IEMobile)]><html class="ie7 ie6-7 ie6-8" xmlns="http://www.w3.org/1999/xhtml" lang="ru" xml:lang="ru" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if IE 8]><html class="ie8 ie6-8" xmlns="http://www.w3.org/1999/xhtml" lang="ru" xml:lang="ru" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><![endif]--> <!--[if (gte IE 9)|(gt IEMobile 7)]><!--><html xmlns="http://www.w3.org/1999/xhtml" lang="ru" xml:lang="ru" xmlns:og="http://ogp.me/ns#" xmlns:fb="http://ogp.me/ns/fb#"><!--<![endif]--> <head> <title>Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts - CERN Document Server</title> <link href='https://framework.web.cern.ch/framework/2.0/fonts/PTSansWeb/PTSansWeb.css' rel='stylesheet' type='text/css' /> <link rel="stylesheet" href="https://cds.cern.ch/img/invenio.css?v=20141127" type="text/css" /> <link rel="stylesheet" href="https://cds.cern.ch/img/cern_theme/css/cern_theme.css?v=20141127" type="text/css" /> <link rel="stylesheet"href="/css/font-awesome.min.css"> <meta http-equiv="X-UA-Compatible" content="IE=Edge"/> <link rel="stylesheet" href="https://cds.cern.ch/img/cern_toolbar/css/toolbar.css" type="text/css" /> <!--[if lt IE 8]> <link href="https://cds.cern.ch/img/cern_toolbar/css/toolbar-ie.css" rel="stylesheet" type="text/css"> <![endif]--> <!--[if lt IE 8]> <link rel="stylesheet" type="text/css" href="https://cds.cern.ch/img/invenio-ie7.css" /> <![endif]--> <!--[if gt IE 8]> <style type="text/css">div.restrictedflag {filter:none;}</style> <![endif]--> <link rel="canonical" href="https://cds.cern.ch/record/1530690" /> <link rel="alternate" hreflang="el" href="https://cds.cern.ch/record/1530690?ln=el" /> <link rel="alternate" hreflang="fr" href="https://cds.cern.ch/record/1530690?ln=fr" /> <link rel="alternate" hreflang="bg" href="https://cds.cern.ch/record/1530690?ln=bg" /> <link rel="alternate" hreflang="zh-TW" href="https://cds.cern.ch/record/1530690?ln=zh_TW" /> <link rel="alternate" hreflang="pt" href="https://cds.cern.ch/record/1530690?ln=pt" /> <link rel="alternate" hreflang="no" href="https://cds.cern.ch/record/1530690?ln=no" /> <link rel="alternate" hreflang="hr" href="https://cds.cern.ch/record/1530690?ln=hr" /> <link rel="alternate" hreflang="ca" href="https://cds.cern.ch/record/1530690?ln=ca" /> <link rel="alternate" hreflang="de" href="https://cds.cern.ch/record/1530690?ln=de" /> <link rel="alternate" hreflang="it" href="https://cds.cern.ch/record/1530690?ln=it" /> <link rel="alternate" hreflang="zh-CN" href="https://cds.cern.ch/record/1530690?ln=zh_CN" /> <link rel="alternate" hreflang="sv" href="https://cds.cern.ch/record/1530690?ln=sv" /> <link rel="alternate" hreflang="sk" href="https://cds.cern.ch/record/1530690?ln=sk" /> <link rel="alternate" hreflang="en" href="https://cds.cern.ch/record/1530690?ln=en" /> <link rel="alternate" hreflang="pl" href="https://cds.cern.ch/record/1530690?ln=pl" /> <link rel="alternate" hreflang="ru" href="https://cds.cern.ch/record/1530690?ln=ru" /> <link rel="alternate" hreflang="ka" href="https://cds.cern.ch/record/1530690?ln=ka" /> <link rel="alternate" hreflang="ja" href="https://cds.cern.ch/record/1530690?ln=ja" /> <link rel="alternate" hreflang="es" href="https://cds.cern.ch/record/1530690?ln=es" /> <link rel="alternate" type="application/rss+xml" title="CERN Document Server RSS" href="/rss?ln=ru" /> <link rel="search" type="application/opensearchdescription+xml" href="https://cds.cern.ch/opensearchdescription" title="CERN Document Server" /> <link rel="unapi-server" type="application/xml" title="unAPI" href="https://cds.cern.ch/unapi" /> <link rel="apple-touch-icon" href="/apple-touch-icon.png"/> <link rel="apple-touch-icon-precomposed" href="/apple-touch-icon-precomposed.png"/> <meta http-equiv="Content-Type" content="text/html; charset=utf-8" /> <meta http-equiv="Content-Language" content="ru" /> <meta name="description" content="We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev--Zeldovich (SZ) effect, and the sub-sample used here has a signal-to-noise threshold of seven, with each object confirmed as a cluster and all but one with a redshift estimate. We discuss the completeness of the sample and our construction of a likelihood analysis. Using a relation between mass $M$ and SZ signal $Y$ calibrated to X-ray measurements, we derive constraints on the power spectrum amplitude $\sigma_8$ and matter density parameter $\Omega_{\mathrm{m}}$ in a flat $\Lambda$CDM model. We test the robustness of our estimates and find that possible biases in the $Y$--$M$ relation and the halo mass function are larger than the statistical uncertainties from the cluster sample. Assuming the X-ray determined mass to be biased low relative to the true mass by between zero and 30%, motivated by comparison of the observed mass scaling relations to those from a set of numerical simulations, we find that $\sigma_8=0.75\pm 0.03$, $\Omega_{\mathrm{m}}=0.29\pm 0.02$, and $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3} = 0.764 \pm 0.025$. The value of $\sigma_8$ is degenerate with the mass bias; if the latter is fixed to a value of 20% we find $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3}=0.78\pm 0.01$ and a tighter one-dimensional range $\sigma_8=0.77\pm 0.02$. We find that the larger values of $\sigma_8$ and $\Omega_{\mathrm{m}}$ preferred by Planck's measurements of the primary CMB anisotropies can be accommodated by a mass bias of about 40%. Alternatively, consistency with the primary CMB constraints can be achieved by inclusion of processes that suppress power on small scales relative to the $\Lambda$CDM model, such as a component of massive neutrinos (abridged). We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev--Zeldovich (SZ) effect, and the sub-sample used here has a signal-to-noise threshold of seven, with each object confirmed as a cluster and all but one with a redshift estimate. We discuss the completeness of the sample and our construction of a likelihood analysis. Using a relation between mass $M$ and SZ signal $Y$ calibrated to X-ray measurements, we derive constraints on the power spectrum amplitude $\sigma_8$ and matter density parameter $\Omega_{\mathrm{m}}$ in a flat $\Lambda$CDM model. We test the robustness of our estimates and find that possible biases in the $Y$--$M$ relation and the halo mass function are larger than the statistical uncertainties from the cluster sample. Assuming the X-ray determined mass to be biased low relative to the true mass by between zero and 30%, motivated by comparison of the observed mass scaling relations to those from a set of numerical simulations, we find that $\sigma_8=0.75\pm 0.03$, $\Omega_{\mathrm{m}}=0.29\pm 0.02$, and $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3} = 0.764 \pm 0.025$. The value of $\sigma_8$ is degenerate with the mass bias; if the latter is fixed to a value of 20% we find $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3}=0.78\pm 0.01$ and a tighter one-dimensional range $\sigma_8=0.77\pm 0.02$. We find that the larger values of $\sigma_8$ and $\Omega_{\mathrm{m}}$ preferred by Planck's measurements of the primary CMB anisotropies can be accommodated by a mass bias of about 40%. Alternatively, consistency with the primary CMB constraints can be achieved by inclusion of processes that suppress power on small scales relative to the $\Lambda$CDM model, such as a component of massive neutrinos (abridged). Ade, P.A.R.; Aghanim, N.; Armitage-Caplan, C.; Arnaud, M.; Ashdown, M.; Atrio-Barandela, F.; Aumont, J.; Baccigalupi, C.; Banday, A.J.; Barreiro, R.B.; Barrena, R.; Bartlett, J.G.; Battaner, E.; Battye, R.; Benabed, K.; Benoit, A.; Benoit-Levy, A.; Bernard, J.P.; Bersanelli, M.; Bielewicz, P.; Bikmaev, I.; Blanchard, A.; Bobin, J.; Bock, J.J.; Bohringer, H.; Bonaldi, A.; Bond, J.R.; Borrill, J.; Bouchet, F.R.; Bourdin, H.; Bridges, M.; Brown, M.L.; Bucher, M.; Burenin, R.; Burigana, C.; Butler, R.C.; Cardoso, J.F.; Carvalho, P.; Catalano, A.; Challinor, A.; Chamballu, A.; Chary, R.R.; Chiang, L.Y.; Chiang, H.C.; Chon, G.; Christensen, P.R.; Church, S.; Clements, D.L.; Colombi, S.; Colombo, L.P.L.; Couchot, F.; Coulais, A.; Crill, B.P.; Curto, A.; Cuttaia, F.; Da Silva, A.; Dahle, H.; Danese, L.; Davies, R.D.; Davis, R.J.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; Delabrouille, J.; Delouis, J.M.; Democles, J.; Desert, F.X.; Dickinson, C.; Diego, J.M.; Dolag, K.; Dole, H.; Donzelli, S.; Dore, O.; Douspis, M.; Dupac, X.; Efstathiou, G.; Ensslin, T.A.; Eriksen, H.K.; Finelli, F.; Flores-Cacho, I.; Forni, O.; Frailis, M.; Franceschi, E.; Fromenteau, S.; Galeotta, S.; Ganga, K.; Genova-Santos, R.T.; Giard, M.; Giardino, G.; Giraud-Heraud, Y.; Gonzalez-Nuevo, J.; Gorski, K.M.; Gratton, S.; Gregorio, A.; Gruppuso, A.; Hansen, F.K.; Hanson, D.; Harrison, D.; Henrot-Versille, S.; Hernandez-Monteagudo, C.; Herranz, D.; Hildebrandt, S.R.; Hivon, E.; Hobson, M.; Holmes, W.A.; Hornstrup, A.; Hovest, W.; Huffenberger, K.M.; Hurier, G.; Jaffe, T.R.; Jaffe, A.H.; Jones, W.C.; Juvela, M.; Keihanen, E.; Keskitalo, R.; Khamitov, I.; Kisner, T.S.; Kneissl, R.; Knoche, J.; Knox, L.; Kunz, M.; Kurki-Suonio, H.; Lagache, G.; Lahteenmaki, A.; Lamarre, J.M.; Lasenby, A.; Laureijs, R.J.; Lawrence, C.R.; Leahy, J.P.; Leonardi, R.; Leon-Tavares, J.; Lesgourgues, J.; Liddle, A.; Liguori, M.; Lilje, P.B.; Linden-Vornle, M.; Lopez-Caniego, M.; Lubin, P.M.; Macias-Perez, J.F.; Maffei, B.; Maino, D.; Mandolesi, N.; Marcos-Caballero, A.; Maris, M.; Marshall, D.J.; Martin, P.G.; Martinez-Gonzalez, E.; Masi, S.; Matarrese, S.; Matthai, F.; Mazzotta, P.; Meinhold, P.R.; Melchiorri, A.; Melin, J.B.; Mendes, L.; Mennella, A.; Migliaccio, M.; Mitra, S.; Miville-Deschenes, M.A.; Moneti, A.; Montier, L.; Morgante, G.; Mortlock, D.; Moss, A.; Munshi, D.; Naselsky, P.; Nati, F.; Natoli, P.; Netterfield, C.B.; Norgaard-Nielsen, H.U.; Noviello, F.; Novikov, D.; Novikov, I.; Osborne, S.; Oxborrow, C.A.; Paci, F.; Pagano, L.; Pajot, F.; Paoletti, D.; Partridge, B.; Pasian, F.; Patanchon, G.; Perdereau, O.; Perotto, L.; Perrotta, F.; Piacentini, F.; Piat, M.; Pierpaoli, E.; Pietrobon, D.; Plaszczynski, S.; Pointecouteau, E.; Polenta, G.; Ponthieu, N.; Popa, L.; Poutanen, T.; Pratt, G.W.; Prezeau, G.; Prunet, S.; Puget, J.L.; Rachen, J.P.; Rebolo, R.; Reinecke, M.; Remazeilles, M.; Renault, C.; Ricciardi, S.; Riller, T.; Ristorcelli, I.; Rocha, G.; Roman, M.; Rosset, C.; Roudier, G.; Rowan-Robinson, M.; Rubino-Martin, J.A.; Rusholme, B.; Sandri, M.; Santos, D.; Savini, G.; Scott, D.; Seiffert, M.D.; Shellard, E.P.S.; Spencer, L.D.; Starck, J.L.; Stolyarov, V.; Stompor, R.; Sudiwala, R.; Sunyaev, R.; Sureau, F.; Sutton, D.; Suur-Uski, A.S.; Sygnet, J.F.; Tauber, J.A.; Tavagnacco, D.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Tristram, M.; Tucci, M.; Tuovinen, J.; Turler, M.; Umana, G.; Valenziano, L.; Valiviita, J.; Van Tent, B.; Vielva, P.; Villa, F.; Vittorio, N.; Wade, L.A.; Wandelt, B.D.; Weller, J.; White, M.; White, S.D.M.; Yvon, D.; Zacchei, A.; Zonca, A." /> <meta name="keywords" content="CERN Document Server, WebSearch, CERN Document Server" /> <script type="text/javascript" src="https://cds.cern.ch/js/jquery.min.js"></script> <!-- WebNews CSS library --> <link rel="stylesheet" href="https://cds.cern.ch/img/webnews.css" type="text/css" /> <!-- WebNews JS library --> <script type="text/javascript" src="https://cds.cern.ch/js/webnews.js?v=20131009"></script> <meta property="fb:app_id" content="137353533001720"/> <script type="text/x-mathjax-config"> MathJax.Hub.Config({ tex2jax: {inlineMath: [['$','$']], processEscapes: true}, showProcessingMessages: false, messageStyle: "none" }); </script> <script src="/MathJax/MathJax.js?config=TeX-AMS_CHTML" type="text/javascript"> </script> <!-- GoogleScholar --> <meta content="Planck 2013 results. 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Astrophys." name="citation_journal_title" /> <meta content="571" name="citation_volume" /> <meta content="A20" name="citation_firstpage" /> <meta content="2013/03/22" name="citation_publication_date" /> <meta name="citation_online_date" content="2013/03/23"> <meta content="astro-ph.CO" name="citation_keywords" /> <meta content="CERN-PH-TH-2013-133" name="citation_technical_report_number" /> <meta content="arXiv:1303.5080" name="citation_technical_report_number" /> <meta content="CERN-PH-TH-2013-133" name="citation_technical_report_number" /> <meta content="10.1051/0004-6361/201321521" name="citation_doi" /> <meta name="citation_pdf_url" content="https://cds.cern.ch/record/1530690/files/arXiv:1303.5080.pdf" /> <!-- OpenGraph --> <meta content="Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts" property="og:title" /> <meta content="website" property="og:type" /> <meta content="https://cds.cern.ch/record/1530690" property="og:url" /> <meta name="twitter:image" content="https://cds.cern.ch/record/1530690/files/Figures_cosmo_sample.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_cosmo_sample.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_cosmo_sample.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_C_OSbnH_BAO_MMF1reorder_2D_pp.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_C_OSbnH_BAO_MMF1reorder_2D_pp.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_counts.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_counts.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_noisemap.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_noisemap.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_figA1.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_figA1.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_completeness.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_completeness.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_sigma8.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_sigma8.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_Mlim4.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_Mlim4.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_comp_ratio.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_comp_ratio.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_NEW-base_planck_lowl_lowLike_reorder_2D.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_NEW-base_planck_lowl_lowLike_reorder_2D.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_comp_scal.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_comp_scal.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_CPPP_old_C_OSbnH_BAO_on_MMF37_watson_2D_PP.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_CPPP_old_C_OSbnH_BAO_on_MMF37_watson_2D_PP.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/fig00005.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/fig00005.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_lpbvsM.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_lpbvsM.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_snr.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_snr.png" /> <meta property="og:image" content="https://cds.cern.ch/record/1530690/files/Figures_pneutrinos.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/1530690/files/Figures_pneutrinos.png" /> <meta content="CERN Document Server" property="og:site_name" /> <meta content="We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev--Zeldovich (SZ) effect, and the sub-sample used here has a signal-to-noise threshold of seven, with each object confirmed as a cluster and all but one with a redshift estimate. We discuss the completeness of the sample and our construction of a likelihood analysis. Using a relation between mass $M$ and SZ signal $Y$ calibrated to X-ray measurements, we derive constraints on the power spectrum amplitude $\sigma_8$ and matter density parameter $\Omega_{\mathrm{m}}$ in a flat $\Lambda$CDM model. We test the robustness of our estimates and find that possible biases in the $Y$--$M$ relation and the halo mass function are larger than the statistical uncertainties from the cluster sample. Assuming the X-ray determined mass to be biased low relative to the true mass by between zero and 30%, motivated by comparison of the observed mass scaling relations to those from a set of numerical simulations, we find that $\sigma_8=0.75\pm 0.03$, $\Omega_{\mathrm{m}}=0.29\pm 0.02$, and $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3} = 0.764 \pm 0.025$. The value of $\sigma_8$ is degenerate with the mass bias; if the latter is fixed to a value of 20% we find $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3}=0.78\pm 0.01$ and a tighter one-dimensional range $\sigma_8=0.77\pm 0.02$. We find that the larger values of $\sigma_8$ and $\Omega_{\mathrm{m}}$ preferred by Planck's measurements of the primary CMB anisotropies can be accommodated by a mass bias of about 40%. 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XX. Cosmology from Sunyaev-Zeldovich cluster counts </td> </tr> </table> </div> <div class="pagebody"><div class="pagebodystripemiddle"> <div class="detailedrecordbox"> <div class="detailedrecordtabs"> <div> <ul class="detailedrecordtabs"><li class="on first"><a href="/record/1530690/?ln=ru">Информация </a></li><li class=""><a href="/record/1530690/files?ln=ru">Файлы </a></li></ul> <div id="tabsSpacer" style="clear:both;height:0px"> </div></div> </div> <div class="detailedrecordboxcontent"> <div class="top-left-folded"></div> <div class="top-right-folded"></div> <div class="inside"> <!--<div style="height:0.1em;"> </div> <p class="notopgap"> </p>--> <abbr class="unapi-id" title="1530690"></abbr> <style type="text/css"> <!-- ul.detailedrecordtabs li.on a{background-color:#4D94CC;color:#fff !important;border-bottom:1px solid #4D94CC!important;} div.detailedrecordboxcontent {padding-top:0px !important;} --> </style> <table class="formatRecordTableFullWidth" > <tr> <td class="formatRecordHeader" style="background-image: url('https://cds.cern.ch/img/journals.jpg');" colspan="2"> <!--YTD: record may have more than one 690C.a tag--> Article </td> </tr> <script type="text/javascript"> $( document ).ready(function() { $('.showAuthor').on('click', function() { var author = '<p>' + $(this).data('name') + '</p>'; var affiliation = $(this).data('affiliation') + '</br>'; var contribution = $(this).data('contribution') + '</br>'; $.magnificPopup.open({ items: { src: '<div id="ovelary-mathjax" class="overlay-white oc-content overlay-white-500">' + author + affiliation + contribution + '</div>', type: 'inline' }, callbacks: { open: function() { var div = document.getElementById("overlay-mathjax") MathJax.Hub.Queue(["Typeset", MathJax.Hub, div]); }, } }) }) }); </script> <tr><td class="formatRecordLabel"> Report number </td><td style="padding-left:5px;"><a href="http://arxiv.org/abs/arXiv:1303.5080">arXiv:1303.5080</a> ; CERN-PH-TH-2013-133 ; CERN-PH-TH-2013-133</td></tr> <tr><td class="formatRecordLabel"> Title </td><td style="padding-left:5px;"><b>Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts</b></td></tr> <tr><td class="formatRecordLabel"><span style="white-space:nowrap;"> Author(s) </span> </td><td style="padding-left:5px;"> <script type="text/javascript"> function toggle_authors_visibility(){ var more = document.getElementById('more'); var link = document.getElementById('link'); var extension = document.getElementById('extension'); if (more.style.display=='none'){ more.style.display = ''; extension.style.display = 'none'; link.innerHTML = "Руководство" } else { more.style.display = 'none'; extension.style.display = ''; link.innerHTML = "Показать всех 254 авторов" } link.style.color = "rgb(204,0,0);" } function set_up(){ var extension = document.getElementById('extension'); extension.innerHTML = "Planck Collaboration "; toggle_authors_visibility(); } </script> <a name="show_hide" /><p id="more" style=""><a href="https://cds.cern.ch/search?f=author&p=Ade%2C%20P.A.R.&ln=ru">Ade, P.A.R.</a> (Cardiff U.) ; <a href="https://cds.cern.ch/search?f=author&p=Aghanim%2C%20N.&ln=ru">Aghanim, N.</a> (Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Armitage-Caplan%2C%20C.&ln=ru">Armitage-Caplan, C.</a> (Oxford U.) ; <a href="https://cds.cern.ch/search?f=author&p=Arnaud%2C%20M.&ln=ru">Arnaud, M.</a> (DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Ashdown%2C%20M.&ln=ru">Ashdown, M.</a> (Cambridge U. ; Cambridge U., KICC) ; <a href="https://cds.cern.ch/search?f=author&p=Atrio-Barandela%2C%20F.&ln=ru">Atrio-Barandela, F.</a> (Salamanca U.) ; <a href="https://cds.cern.ch/search?f=author&p=Aumont%2C%20J.&ln=ru">Aumont, J.</a> (Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Baccigalupi%2C%20C.&ln=ru">Baccigalupi, C.</a> (SISSA, Trieste) ; <a href="https://cds.cern.ch/search?f=author&p=Banday%2C%20A.J.&ln=ru">Banday, A.J.</a> (IRAP, Toulouse ; Toulouse III U.) ; <a href="https://cds.cern.ch/search?f=author&p=Barreiro%2C%20R.B.&ln=ru">Barreiro, R.B.</a> (Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Barrena%2C%20R.&ln=ru">Barrena, R.</a> (IAC, La Laguna) ; <a href="https://cds.cern.ch/search?f=author&p=Bartlett%2C%20J.G.&ln=ru">Bartlett, J.G.</a> (Caltech ; APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Battaner%2C%20E.&ln=ru">Battaner, E.</a> (Granada U.) ; <a href="https://cds.cern.ch/search?f=author&p=Battye%2C%20R.&ln=ru">Battye, R.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Benabed%2C%20K.&ln=ru">Benabed, K.</a> (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Benoit%2C%20A.&ln=ru">Benoit, A.</a> (LPSC, Grenoble) ; <a href="https://cds.cern.ch/search?f=author&p=Benoit-Levy%2C%20A.&ln=ru">Benoit-Levy, A.</a> (Paris U., VI-VII ; Paris, Inst. Astrophys. ; University Coll. London) ; <a href="https://cds.cern.ch/search?f=author&p=Bernard%2C%20J.P.&ln=ru">Bernard, J.P.</a> (IRAP, Toulouse) ; <a href="https://cds.cern.ch/search?f=author&p=Bersanelli%2C%20M.&ln=ru">Bersanelli, M.</a> (Brera Observ. ; Milan U.) ; <a href="https://cds.cern.ch/search?f=author&p=Bielewicz%2C%20P.&ln=ru">Bielewicz, P.</a> (SISSA, Trieste ; IRAP, Toulouse ; Toulouse III U.) ; <a href="https://cds.cern.ch/search?f=author&p=Bikmaev%2C%20I.&ln=ru">Bikmaev, I.</a> (Acad. Sci. of Tatarstan ; Kazan State U.) ; <a href="https://cds.cern.ch/search?f=author&p=Blanchard%2C%20A.&ln=ru">Blanchard, A.</a> (Toulouse III U.) ; <a href="https://cds.cern.ch/search?f=author&p=Bobin%2C%20J.&ln=ru">Bobin, J.</a> (DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Bock%2C%20J.J.&ln=ru">Bock, J.J.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Bohringer%2C%20H.&ln=ru">Bohringer, H.</a> (Garching, Max Planck Inst., MPE) ; <a href="https://cds.cern.ch/search?f=author&p=Bonaldi%2C%20A.&ln=ru">Bonaldi, A.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Bond%2C%20J.R.&ln=ru">Bond, J.R.</a> (Canadian Inst. Theor. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Borrill%2C%20J.&ln=ru">Borrill, J.</a> (UC, Berkeley ; LBL, Berkeley) ; <a href="https://cds.cern.ch/search?f=author&p=Bouchet%2C%20F.R.&ln=ru">Bouchet, F.R.</a> (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Bourdin%2C%20H.&ln=ru">Bourdin, H.</a> (Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Bridges%2C%20M.&ln=ru">Bridges, M.</a> (Cambridge U., Inst. of Astron. ; Cambridge U. ; Cambridge U., KICC) ; <a href="https://cds.cern.ch/search?f=author&p=Brown%2C%20M.L.&ln=ru">Brown, M.L.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Bucher%2C%20M.&ln=ru">Bucher, M.</a> (APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Burenin%2C%20R.&ln=ru">Burenin, R.</a> (Moscow, MIPT ; Moscow, Space Res. Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Burigana%2C%20C.&ln=ru">Burigana, C.</a> (Ferrara U. ; Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Butler%2C%20R.C.&ln=ru">Butler, R.C.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Cardoso%2C%20J.F.&ln=ru">Cardoso, J.F.</a> (Paris, Inst. Astrophys. ; APC, Paris ; LTCI, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Carvalho%2C%20P.&ln=ru">Carvalho, P.</a> (Cambridge U.) ; <a href="https://cds.cern.ch/search?f=author&p=Catalano%2C%20A.&ln=ru">Catalano, A.</a> (LERMA, Ivry ; LPSC, Grenoble) ; <a href="https://cds.cern.ch/search?f=author&p=Challinor%2C%20A.&ln=ru">Challinor, A.</a> (Cambridge U., DAMTP ; Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; <a href="https://cds.cern.ch/search?f=author&p=Chamballu%2C%20A.&ln=ru">Chamballu, A.</a> (Paris, Inst. Astrophys. ; DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Chary%2C%20R.R.&ln=ru">Chary, R.R.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Chiang%2C%20L.Y.&ln=ru">Chiang, L.Y.</a> (Taipei, Inst. Astron. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Chiang%2C%20H.C.&ln=ru">Chiang, H.C.</a> (KwaZulu Natal U. ; Princeton U.) ; <a href="https://cds.cern.ch/search?f=author&p=Chon%2C%20G.&ln=ru">Chon, G.</a> (Garching, Max Planck Inst., MPE) ; <a href="https://cds.cern.ch/search?f=author&p=Christensen%2C%20P.R.&ln=ru">Christensen, P.R.</a> (Bohr Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Church%2C%20S.&ln=ru">Church, S.</a> (Stanford U., Phys. Dept.) ; <a href="https://cds.cern.ch/search?f=author&p=Clements%2C%20D.L.&ln=ru">Clements, D.L.</a> (Imperial Coll., London) ; <a href="https://cds.cern.ch/search?f=author&p=Colombi%2C%20S.&ln=ru">Colombi, S.</a> (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Colombo%2C%20L.P.L.&ln=ru">Colombo, L.P.L.</a> (Caltech ; UCLA) ; <a href="https://cds.cern.ch/search?f=author&p=Couchot%2C%20F.&ln=ru">Couchot, F.</a> (Orsay, LAL) ; <a href="https://cds.cern.ch/search?f=author&p=Coulais%2C%20A.&ln=ru">Coulais, A.</a> (LERMA, Ivry) ; <a href="https://cds.cern.ch/search?f=author&p=Crill%2C%20B.P.&ln=ru">Crill, B.P.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Curto%2C%20A.&ln=ru">Curto, A.</a> (Cantabria Inst. of Phys. ; Cambridge U.) ; <a href="https://cds.cern.ch/search?f=author&p=Cuttaia%2C%20F.&ln=ru">Cuttaia, F.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Da%20Silva%2C%20A.&ln=ru">Da Silva, A.</a> (Porto U., Astron. Dept.) ; <a href="https://cds.cern.ch/search?f=author&p=Dahle%2C%20H.&ln=ru">Dahle, H.</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Danese%2C%20L.&ln=ru">Danese, L.</a> (SISSA, Trieste) ; <a href="https://cds.cern.ch/search?f=author&p=Davies%2C%20R.D.&ln=ru">Davies, R.D.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Davis%2C%20R.J.&ln=ru">Davis, R.J.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=de%20Bernardis%2C%20P.&ln=ru">de Bernardis, P.</a> (Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=de%20Rosa%2C%20A.&ln=ru">de Rosa, A.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=de%20Zotti%2C%20G.&ln=ru">de Zotti, G.</a> (SISSA, Trieste ; Padua Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Delabrouille%2C%20J.&ln=ru">Delabrouille, J.</a> (APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Delouis%2C%20J.M.&ln=ru">Delouis, J.M.</a> (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Democles%2C%20J.&ln=ru">Democles, J.</a> (DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Desert%2C%20F.X.&ln=ru">Desert, F.X.</a> (Grenoble Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Dickinson%2C%20C.&ln=ru">Dickinson, C.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Diego%2C%20J.M.&ln=ru">Diego, J.M.</a> (Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Dolag%2C%20K.&ln=ru">Dolag, K.</a> (Garching, Max Planck Inst. ; Munich U.) ; <a href="https://cds.cern.ch/search?f=author&p=Dole%2C%20H.&ln=ru">Dole, H.</a> (IUF, Paris ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Donzelli%2C%20S.&ln=ru">Donzelli, S.</a> (Brera Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Dore%2C%20O.&ln=ru">Dore, O.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Douspis%2C%20M.&ln=ru">Douspis, M.</a> (Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Dupac%2C%20X.&ln=ru">Dupac, X.</a> (ESA, Madrid) ; <a href="https://cds.cern.ch/search?f=author&p=Efstathiou%2C%20G.&ln=ru">Efstathiou, G.</a> (Cambridge U., Inst. of Astron.) ; <a href="https://cds.cern.ch/search?f=author&p=Ensslin%2C%20T.A.&ln=ru">Ensslin, T.A.</a> (Garching, Max Planck Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Eriksen%2C%20H.K.&ln=ru">Eriksen, H.K.</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Finelli%2C%20F.&ln=ru">Finelli, F.</a> (INFN, Bologna ; Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Flores-Cacho%2C%20I.&ln=ru">Flores-Cacho, I.</a> (Toulouse III U. ; IRAP, Toulouse) ; <a href="https://cds.cern.ch/search?f=author&p=Forni%2C%20O.&ln=ru">Forni, O.</a> (IRAP, Toulouse ; Toulouse III U.) ; <a href="https://cds.cern.ch/search?f=author&p=Frailis%2C%20M.&ln=ru">Frailis, M.</a> (Trieste Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Franceschi%2C%20E.&ln=ru">Franceschi, E.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Fromenteau%2C%20S.&ln=ru">Fromenteau, S.</a> (Paris, Inst. Astrophys. ; APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Galeotta%2C%20S.&ln=ru">Galeotta, S.</a> (Trieste Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Ganga%2C%20K.&ln=ru">Ganga, K.</a> (APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Genova-Santos%2C%20R.T.&ln=ru">Genova-Santos, R.T.</a> (IAC, La Laguna) ; <a href="https://cds.cern.ch/search?f=author&p=Giard%2C%20M.&ln=ru">Giard, M.</a> (IRAP, Toulouse ; Toulouse III U.) ; <a href="https://cds.cern.ch/search?f=author&p=Giardino%2C%20G.&ln=ru">Giardino, G.</a> (ESTEC, Noordwijk) ; <a href="https://cds.cern.ch/search?f=author&p=Giraud-Heraud%2C%20Y.&ln=ru">Giraud-Heraud, Y.</a> (APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Gonzalez-Nuevo%2C%20J.&ln=ru">Gonzalez-Nuevo, J.</a> (SISSA, Trieste ; Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Gorski%2C%20K.M.&ln=ru">Gorski, K.M.</a> (Warsaw U. ; Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Gratton%2C%20S.&ln=ru">Gratton, S.</a> (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; <a href="https://cds.cern.ch/search?f=author&p=Gregorio%2C%20A.&ln=ru">Gregorio, A.</a> (Trieste Observ. ; Trieste U.) ; <a href="https://cds.cern.ch/search?f=author&p=Gruppuso%2C%20A.&ln=ru">Gruppuso, A.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Hansen%2C%20F.K.&ln=ru">Hansen, F.K.</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Hanson%2C%20D.&ln=ru">Hanson, D.</a> (Canadian Inst. Theor. Astrophys. ; Caltech ; Rutherford) ; <a href="https://cds.cern.ch/search?f=author&p=Harrison%2C%20D.&ln=ru">Harrison, D.</a> (Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; <a href="https://cds.cern.ch/search?f=author&p=Henrot-Versille%2C%20S.&ln=ru">Henrot-Versille, S.</a> (Orsay, LAL) ; <a href="https://cds.cern.ch/search?f=author&p=Hernandez-Monteagudo%2C%20C.&ln=ru">Hernandez-Monteagudo, C.</a> (Garching, Max Planck Inst. ; CEFCA, Teruel) ; <a href="https://cds.cern.ch/search?f=author&p=Herranz%2C%20D.&ln=ru">Herranz, D.</a> (Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Hildebrandt%2C%20S.R.&ln=ru">Hildebrandt, S.R.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Hivon%2C%20E.&ln=ru">Hivon, E.</a> (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Hobson%2C%20M.&ln=ru">Hobson, M.</a> (Cambridge U.) ; <a href="https://cds.cern.ch/search?f=author&p=Holmes%2C%20W.A.&ln=ru">Holmes, W.A.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Hornstrup%2C%20A.&ln=ru">Hornstrup, A.</a> (Denmark, Tech. U.) ; <a href="https://cds.cern.ch/search?f=author&p=Hovest%2C%20W.&ln=ru">Hovest, W.</a> (Garching, Max Planck Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Huffenberger%2C%20K.M.&ln=ru">Huffenberger, K.M.</a> (Miami U.) ; <a href="https://cds.cern.ch/search?f=author&p=Hurier%2C%20G.&ln=ru">Hurier, G.</a> (LPSC, Grenoble ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Jaffe%2C%20T.R.&ln=ru">Jaffe, T.R.</a> (IRAP, Toulouse ; Toulouse III U.) ; <a href="https://cds.cern.ch/search?f=author&p=Jaffe%2C%20A.H.&ln=ru">Jaffe, A.H.</a> (Imperial Coll., London) ; <a href="https://cds.cern.ch/search?f=author&p=Jones%2C%20W.C.&ln=ru">Jones, W.C.</a> (Princeton U.) ; <a href="https://cds.cern.ch/search?f=author&p=Juvela%2C%20M.&ln=ru">Juvela, M.</a> (Helsinki U.) ; <a href="https://cds.cern.ch/search?f=author&p=Keihanen%2C%20E.&ln=ru">Keihanen, E.</a> (Helsinki U.) ; <a href="https://cds.cern.ch/search?f=author&p=Keskitalo%2C%20R.&ln=ru">Keskitalo, R.</a> (LBL, Berkeley ; UC, Berkeley) ; <a href="https://cds.cern.ch/search?f=author&p=Khamitov%2C%20I.&ln=ru">Khamitov, I.</a> (Kazan State U. ; Akdeniz U.) ; <a href="https://cds.cern.ch/search?f=author&p=Kisner%2C%20T.S.&ln=ru">Kisner, T.S.</a> (LBL, Berkeley) ; <a href="https://cds.cern.ch/search?f=author&p=Kneissl%2C%20R.&ln=ru">Kneissl, R.</a> (European Southern Obs., Chile) ; <a href="https://cds.cern.ch/search?f=author&p=Knoche%2C%20J.&ln=ru">Knoche, J.</a> (Garching, Max Planck Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Knox%2C%20L.&ln=ru">Knox, L.</a> (UC, Davis) ; <a href="https://cds.cern.ch/search?f=author&p=Kunz%2C%20M.&ln=ru">Kunz, M.</a> (African Inst. Math. Sci., Cape Town ; Paris, Inst. Astrophys. ; Geneva U.) ; <a href="https://cds.cern.ch/search?f=author&p=Kurki-Suonio%2C%20H.&ln=ru">Kurki-Suonio, H.</a> (Helsinki Inst. of Phys. ; Helsinki U.) ; <a href="https://cds.cern.ch/search?f=author&p=Lagache%2C%20G.&ln=ru">Lagache, G.</a> (Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Lahteenmaki%2C%20A.&ln=ru">Lahteenmaki, A.</a> (Helsinki Inst. of Phys. ; Aalto U.) ; <a href="https://cds.cern.ch/search?f=author&p=Lamarre%2C%20J.M.&ln=ru">Lamarre, J.M.</a> (LERMA, Ivry) ; <a href="https://cds.cern.ch/search?f=author&p=Lasenby%2C%20A.&ln=ru">Lasenby, A.</a> (Cambridge U., KICC ; Cambridge U.) ; <a href="https://cds.cern.ch/search?f=author&p=Laureijs%2C%20R.J.&ln=ru">Laureijs, R.J.</a> (ESTEC, Noordwijk) ; <a href="https://cds.cern.ch/search?f=author&p=Lawrence%2C%20C.R.&ln=ru">Lawrence, C.R.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Leahy%2C%20J.P.&ln=ru">Leahy, J.P.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Leonardi%2C%20R.&ln=ru">Leonardi, R.</a> (ESA, Madrid) ; <a href="https://cds.cern.ch/search?f=author&p=Leon-Tavares%2C%20J.&ln=ru">Leon-Tavares, J.</a> (Aalto U. ; Turku U.) ; <a href="https://cds.cern.ch/search?f=author&p=Lesgourgues%2C%20J.&ln=ru">Lesgourgues, J.</a> (LPHE, Lausanne ; CERN) ; <a href="https://cds.cern.ch/search?f=author&p=Liddle%2C%20A.&ln=ru">Liddle, A.</a> (Sussex U. ; Royal Observ., Edinburgh) ; <a href="https://cds.cern.ch/search?f=author&p=Liguori%2C%20M.&ln=ru">Liguori, M.</a> (Padua U.) ; <a href="https://cds.cern.ch/search?f=author&p=Lilje%2C%20P.B.&ln=ru">Lilje, P.B.</a> (Oslo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Linden-Vornle%2C%20M.&ln=ru">Linden-Vornle, M.</a> (Denmark, Tech. U.) ; <a href="https://cds.cern.ch/search?f=author&p=Lopez-Caniego%2C%20M.&ln=ru">Lopez-Caniego, M.</a> (Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Lubin%2C%20P.M.&ln=ru">Lubin, P.M.</a> (UC, Santa Barbara) ; <a href="https://cds.cern.ch/search?f=author&p=Macias-Perez%2C%20J.F.&ln=ru">Macias-Perez, J.F.</a> (LPSC, Grenoble) ; <a href="https://cds.cern.ch/search?f=author&p=Maffei%2C%20B.&ln=ru">Maffei, B.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Maino%2C%20D.&ln=ru">Maino, D.</a> (Brera Observ. ; Milan U.) ; <a href="https://cds.cern.ch/search?f=author&p=Mandolesi%2C%20N.&ln=ru">Mandolesi, N.</a> (Ferrara U. ; ASI, Rome ; Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Marcos-Caballero%2C%20A.&ln=ru">Marcos-Caballero, A.</a> (Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Maris%2C%20M.&ln=ru">Maris, M.</a> (Trieste Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Marshall%2C%20D.J.&ln=ru">Marshall, D.J.</a> (DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Martin%2C%20P.G.&ln=ru">Martin, P.G.</a> (Canadian Inst. Theor. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Martinez-Gonzalez%2C%20E.&ln=ru">Martinez-Gonzalez, E.</a> (Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Masi%2C%20S.&ln=ru">Masi, S.</a> (Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Matarrese%2C%20S.&ln=ru">Matarrese, S.</a> (Padua U.) ; <a href="https://cds.cern.ch/search?f=author&p=Matthai%2C%20F.&ln=ru">Matthai, F.</a> (Garching, Max Planck Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Mazzotta%2C%20P.&ln=ru">Mazzotta, P.</a> (Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Meinhold%2C%20P.R.&ln=ru">Meinhold, P.R.</a> (UC, Santa Barbara) ; <a href="https://cds.cern.ch/search?f=author&p=Melchiorri%2C%20A.&ln=ru">Melchiorri, A.</a> (INFN, Rome ; Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Melin%2C%20J.B.&ln=ru">Melin, J.B.</a> (DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Mendes%2C%20L.&ln=ru">Mendes, L.</a> (ESA, Madrid) ; <a href="https://cds.cern.ch/search?f=author&p=Mennella%2C%20A.&ln=ru">Mennella, A.</a> (Brera Observ. ; Milan U.) ; <a href="https://cds.cern.ch/search?f=author&p=Migliaccio%2C%20M.&ln=ru">Migliaccio, M.</a> (Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; <a href="https://cds.cern.ch/search?f=author&p=Mitra%2C%20S.&ln=ru">Mitra, S.</a> (Caltech ; Pune U.) ; <a href="https://cds.cern.ch/search?f=author&p=Miville-Deschenes%2C%20M.A.&ln=ru">Miville-Deschenes, M.A.</a> (Canadian Inst. Theor. Astrophys. ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Moneti%2C%20A.&ln=ru">Moneti, A.</a> (Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Montier%2C%20L.&ln=ru">Montier, L.</a> (IRAP, Toulouse ; Toulouse III U.) ; <a href="https://cds.cern.ch/search?f=author&p=Morgante%2C%20G.&ln=ru">Morgante, G.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Mortlock%2C%20D.&ln=ru">Mortlock, D.</a> (Imperial Coll., London) ; <a href="https://cds.cern.ch/search?f=author&p=Moss%2C%20A.&ln=ru">Moss, A.</a> (Nottingham U.) ; <a href="https://cds.cern.ch/search?f=author&p=Munshi%2C%20D.&ln=ru">Munshi, D.</a> (Cardiff U.) ; <a href="https://cds.cern.ch/search?f=author&p=Naselsky%2C%20P.&ln=ru">Naselsky, P.</a> (Bohr Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Nati%2C%20F.&ln=ru">Nati, F.</a> (Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Natoli%2C%20P.&ln=ru">Natoli, P.</a> (Bologna Observ. ; ASDC, Frascati ; Ferrara U.) ; <a href="https://cds.cern.ch/search?f=author&p=Netterfield%2C%20C.B.&ln=ru">Netterfield, C.B.</a> (Toronto U.) ; <a href="https://cds.cern.ch/search?f=author&p=Norgaard-Nielsen%2C%20H.U.&ln=ru">Norgaard-Nielsen, H.U.</a> (Denmark, Tech. U.) ; <a href="https://cds.cern.ch/search?f=author&p=Noviello%2C%20F.&ln=ru">Noviello, F.</a> (Manchester U.) ; <a href="https://cds.cern.ch/search?f=author&p=Novikov%2C%20D.&ln=ru">Novikov, D.</a> (Imperial Coll., London) ; <a href="https://cds.cern.ch/search?f=author&p=Novikov%2C%20I.&ln=ru">Novikov, I.</a> (Bohr Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Osborne%2C%20S.&ln=ru">Osborne, S.</a> (Stanford U., Phys. Dept.) ; <a href="https://cds.cern.ch/search?f=author&p=Oxborrow%2C%20C.A.&ln=ru">Oxborrow, C.A.</a> (Denmark, Tech. U.) ; <a href="https://cds.cern.ch/search?f=author&p=Paci%2C%20F.&ln=ru">Paci, F.</a> (SISSA, Trieste) ; <a href="https://cds.cern.ch/search?f=author&p=Pagano%2C%20L.&ln=ru">Pagano, L.</a> (INFN, Rome ; Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Pajot%2C%20F.&ln=ru">Pajot, F.</a> (Paris, Inst. 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London) ; <a href="https://cds.cern.ch/search?f=author&p=Scott%2C%20D.&ln=ru">Scott, D.</a> (British Columbia U.) ; <a href="https://cds.cern.ch/search?f=author&p=Seiffert%2C%20M.D.&ln=ru">Seiffert, M.D.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Shellard%2C%20E.P.S.&ln=ru">Shellard, E.P.S.</a> (Cambridge U., DAMTP) ; <a href="https://cds.cern.ch/search?f=author&p=Spencer%2C%20L.D.&ln=ru">Spencer, L.D.</a> (Cardiff U.) ; <a href="https://cds.cern.ch/search?f=author&p=Starck%2C%20J.L.&ln=ru">Starck, J.L.</a> (DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Stolyarov%2C%20V.&ln=ru">Stolyarov, V.</a> (Stavropol, Astrophys. 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Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Valenziano%2C%20L.&ln=ru">Valenziano, L.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Valiviita%2C%20J.&ln=ru">Valiviita, J.</a> (Oslo U. ; Helsinki U. ; Helsinki Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Van%20Tent%2C%20B.&ln=ru">Van Tent, B.</a> (Orsay, LPT) ; <a href="https://cds.cern.ch/search?f=author&p=Vielva%2C%20P.&ln=ru">Vielva, P.</a> (Cantabria Inst. of Phys.) ; <a href="https://cds.cern.ch/search?f=author&p=Villa%2C%20F.&ln=ru">Villa, F.</a> (Bologna Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Vittorio%2C%20N.&ln=ru">Vittorio, N.</a> (Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Wade%2C%20L.A.&ln=ru">Wade, L.A.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Wandelt%2C%20B.D.&ln=ru">Wandelt, B.D.</a> (Illinois U., Urbana ; Paris U., VI-VII ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Weller%2C%20J.&ln=ru">Weller, J.</a> (Munich U.) ; <a href="https://cds.cern.ch/search?f=author&p=White%2C%20M.&ln=ru">White, M.</a> (UC, Berkeley) ; <a href="https://cds.cern.ch/search?f=author&p=White%2C%20S.D.M.&ln=ru">White, S.D.M.</a> (Garching, Max Planck Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Yvon%2C%20D.&ln=ru">Yvon, D.</a> (DAPNIA, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Zacchei%2C%20A.&ln=ru">Zacchei, A.</a> (Trieste Observ.) ; <a href="https://cds.cern.ch/search?f=author&p=Zonca%2C%20A.&ln=ru">Zonca, A.</a> (UC, Santa Barbara)</p> <span id="extension"></span> <small><i><a id="link" href="#" onclick="toggle_authors_visibility()" style="color:rgb(204,0,0);"></a></i></small><script type="text/javascript">set_up()</script></td></tr> <tr><td class="formatRecordLabel"> Publication </td><td style="padding-left:5px;">2014-10-29</td></tr> <tr><td class="formatRecordLabel"> Imprint </td><td style="padding-left:5px;">22 Mar 2013</td></tr> <tr><td class="formatRecordLabel"> Number of pages </td><td style="padding-left:5px;">20</td></tr> <tr><td class="formatRecordLabel"> Note </td><td style="padding-left:5px;">Comments: 19 pages, submitted to A&A<br />20 pages, accepted for publication by A&A</td></tr> <tr><td class="formatRecordLabel"> In: </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1051/0004-6361/201321521"><i>Astron. Astrophys.</i> 571 (2014) A20</a> </a></td></tr> <tr><td class="formatRecordLabel"> DOI </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1051/0004-6361/201321521" title="DOI" target="_blank">10.1051/0004-6361/201321521</a> <tr><td class="formatRecordLabel"> Subject category </td><td style="padding-left:5px;">Astrophysics and Astronomy</td></tr> <tr><td class="formatRecordLabel"> Accelerator/Facility, Experiment </td><td style="padding-left:5px;"><a href="https://cds.cern.ch/search?p=PLANCK%20RE24&f=693__e">PLANCK RE24</a></td></tr> <tr><td class="formatRecordLabel"> Abstract </td><td style="padding-left:5px;">We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev--Zeldovich (SZ) effect, and the sub-sample used here has a signal-to-noise threshold of seven, with each object confirmed as a cluster and all but one with a redshift estimate. We discuss the completeness of the sample and our construction of a likelihood analysis. Using a relation between mass $M$ and SZ signal $Y$ calibrated to X-ray measurements, we derive constraints on the power spectrum amplitude $\sigma_8$ and matter density parameter $\Omega_{\mathrm{m}}$ in a flat $\Lambda$CDM model. We test the robustness of our estimates and find that possible biases in the $Y$--$M$ relation and the halo mass function are larger than the statistical uncertainties from the cluster sample. Assuming the X-ray determined mass to be biased low relative to the true mass by between zero and 30%, motivated by comparison of the observed mass scaling relations to those from a set of numerical simulations, we find that $\sigma_8=0.75\pm 0.03$, $\Omega_{\mathrm{m}}=0.29\pm 0.02$, and $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3} = 0.764 \pm 0.025$. The value of $\sigma_8$ is degenerate with the mass bias; if the latter is fixed to a value of 20% we find $\sigma_8(\Omega_{\mathrm{m}}/0.27)^{0.3}=0.78\pm 0.01$ and a tighter one-dimensional range $\sigma_8=0.77\pm 0.02$. We find that the larger values of $\sigma_8$ and $\Omega_{\mathrm{m}}$ preferred by Planck's measurements of the primary CMB anisotropies can be accommodated by a mass bias of about 40%. Alternatively, consistency with the primary CMB constraints can be achieved by inclusion of processes that suppress power on small scales relative to the $\Lambda$CDM model, such as a component of massive neutrinos (abridged).</td></tr> <tr><td class="formatRecordLabel"> Copyright/License </td><td style="padding-left:5px;">Preprint: © 2013-2024 CERN (License: <a href="http://creativecommons.org/licenses/by/3.0/">CC-BY-3.0</a>)</td></tr> </table> <br /><div style="max-width:1024px;margin:auto"><div style="overflow-x:auto;display:inline;width:100%;"><a href="/record/1530690/plots#0"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/1530690/files/Figures_cosmo_sample.png" title=" Distribution on the sky of the \Planck\ SZ cluster sub-sample used in this paper, with the 35\% mask overlaid." width="200px"/></a> <a href="/record/1530690/plots#1"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/1530690/files/Figures_snr.png" title=" Blind S/N versus S/N re-extracted at the X-ray position using the X-ray size, for the \texttt{MMF3} detections of \Planck\ clusters that are associated with known X-ray clusters in the reference cosmological sample. In contrast to the blind SZ flux, the blind S/N is in good agreement with S/N measured using X-ray priors." width="200px"/></a> <a href="/record/1530690/plots#2"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/1530690/files/Figures_Mlim4.png" title=" Limiting mass as a function of $z$ for the selection function and noise level computed for three zones (deep, blue; medium, cyan; shallow, green), and on average for the unmasked sky (dashed black)." width="200px"/></a> <a href='/record/1530690/plots'>Show more plots</a></div></div><br /> <br/>Corresponding record in: <a href="http://inspirehep.net/record/1224745">Inspire</a> <small> </small> <br/> <br/><br/><div align="right"><div style="padding-bottom:2px;padding-top:30px;"><span class="moreinfo" style="margin-right:10px;"> <a href="" class="moreinfo">Back to search</a> </span></div></div> <div class="bottom-left-folded"><div class="recordlastmodifiedbox" style="position:relative;margin-left:1px"> Запись создана 2013-03-23, последняя модификация 2024-05-03</div></div> <div class="bottom-right-folded" style="text-align:right;padding-bottom:2px;"> <span class="moreinfo" style="margin-right:10px;"><a href="/search?ln=ru&p=recid%3A1530690&rm=wrd" class="moreinfo">Подобные записи</a></span></div> </div> </div> </div> <br/> <br /> <div class="detailedrecordminipanel"> <div class="top-left"></div><div class="top-right"></div> <div class="inside"> <div id="detailedrecordminipanelfile" style="width:33%;float:left;text-align:center;margin-top:0"> <div><small class="detailedRecordActions">Полный текст:</small> <br /><a href="/record/1530690/files/arXiv:1303.5080.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="Загрузка полного текста"/>PDF</a><br /></div><small class="detailedRecordActions">Внешние ссылки:</small><br /><small><a href="http://arxiv.org/pdf/1303.5080.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="Загрузка полного текста"/>Preprint</a><br /><a href="http://www.aanda.org/articles/aa/pdf/2014/11/aa21521-13.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="Загрузка полного текста"/>EDP Sciences Free Access article</a></small> </div> <div id="detailedrecordminipanelreview" style="width:30%;float:left;text-align:center"> </div> <div id="detailedrecordminipanelactions" style="width:36%;float:right;text-align:right;"> <ul class="detailedrecordactions"> <li><a href="/yourbaskets/add?ln=ru&recid=1530690">Добавить в личную книжную полку</a></li> <li>Экспортировать как <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/hx?ln=ru">BibTeX</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/hm?ln=ru">MARC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/xm?ln=ru">MARCXML</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/xd?ln=ru">DC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/xe?ln=ru">EndNote</a>, <!-- <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/xe8x?ln=ru">EndNote (8-X)</a>,--> <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/xn?ln=ru">NLM</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/1530690/export/xw?ln=ru">RefWorks</a> </li> </ul> <div style='padding-left: 13px;'> <!-- JQuery Bookmark Button BEGIN --> <div id="bookmark"></div> <div id="bookmark_sciencewise"></div> <style type="text/css"> #bookmark_sciencewise, #bookmark {float: left;} #bookmark_sciencewise li {padding: 2px; width: 25px;} #bookmark_sciencewise ul, #bookmark ul {list-style-image: none;} </style> <script type="text/javascript" src="/js/jquery.bookmark.min.js"></script> <style type="text/css">@import "/css/jquery.bookmark.css";</style> <script type="text/javascript">// <![CDATA[ $.bookmark.addSite('sciencewise', 'ScienceWise.info', 'https://cds.cern.ch/img/sciencewise.png', 'en', 'bookmark', 'http://sciencewise.info/bookmarks/1303.5080/add'); $('#bookmark_sciencewise').bookmark({sites: ['sciencewise']}); $('#bookmark').bookmark({ sites: ['facebook', 'twitter', 'linkedin', 'google_plusone'], icons: '/img/bookmarks.png', url: 'https://cds.cern.ch/record/1530690', addEmail: true, title: "Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts", description: "We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev--Zeldovich (SZ) effect, and the sub-sample used here has a signal-to-noise threshold of seven, with each object confirmed as a cluster and all but one with a redshift estimate. We discuss the completeness of the sample and our construction of a likelihood analysis. Using a relation between mass $M$ and SZ signal $Y$ calibrated to X-ray measurements, we derive constraints on the power spectrum amplitude $\\sigma_8$ and matter density parameter $\\Omega_{\\mathrm{m}}$ in a flat $\\Lambda$CDM model. We test the robustness of our estimates and find that possible biases in the $Y$--$M$ relation and the halo mass function are larger than the statistical uncertainties from the cluster sample. Assuming the X-ray determined mass to be biased low relative to the true mass by between zero and 30%, motivated by comparison of the observed mass scaling relations to those from a set of numerical simulations, we find that $\\sigma_8=0.75\\pm 0.03$, $\\Omega_{\\mathrm{m}}=0.29\\pm 0.02$, and $\\sigma_8(\\Omega_{\\mathrm{m}}/0.27)^{0.3} = 0.764 \\pm 0.025$. The value of $\\sigma_8$ is degenerate with the mass bias; if the latter is fixed to a value of 20% we find $\\sigma_8(\\Omega_{\\mathrm{m}}/0.27)^{0.3}=0.78\\pm 0.01$ and a tighter one-dimensional range $\\sigma_8=0.77\\pm 0.02$. We find that the larger values of $\\sigma_8$ and $\\Omega_{\\mathrm{m}}$ preferred by Planck\'s measurements of the primary CMB anisotropies can be accommodated by a mass bias of about 40%. Alternatively, consistency with the primary CMB constraints can be achieved by inclusion of processes that suppress power on small scales relative to the $\\Lambda$CDM model, such as a component of massive neutrinos (abridged)." }); // ]]> </script> <!-- JQuery Bookmark Button END --> </div> </div> <div style="clear:both;margin-bottom: 0;"></div> </div> <div class="bottom-left"></div><div class="bottom-right"></div> </div> </div></div> <footer id="footer" class="pagefooter clearfix"> <!-- replaced page footer --> <div class="pagefooterstripeleft"> CERN Document Server :: <a class="footer" href="https://cds.cern.ch/?ln=ru">Искать</a> :: <a class="footer" href="https://cds.cern.ch/submit?ln=ru">Внести</a> :: <a class="footer" href="https://cds.cern.ch/youraccount/display?ln=ru">Персонализовать</a> :: <a class="footer" href="https://cds.cern.ch/help/?ln=ru">Помощь</a> :: <a class="footer" href="https://cern.service-now.com/service-portal?id=privacy_policy&se=CDS-Service" target="_blank">Privacy Notice</a> <br /> Развиваемое <a class="footer" href="http://invenio-software.org/">Invenio</a> <br /> Поддерживает <a class="footer" href="https://cern.service-now.com/service-portal?id=service_element&name=CDS-Service">CDS Service</a> - Need help? 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