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Overview and the cosmological legacy of Planck - 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" />    <link rel="canonical" href="https://cds.cern.ch/record/2636310" /> <link rel="alternate" hreflang="el" href="https://cds.cern.ch/record/2636310?ln=el" /> <link rel="alternate" hreflang="fr" href="https://cds.cern.ch/record/2636310?ln=fr" /> <link rel="alternate" hreflang="bg" href="https://cds.cern.ch/record/2636310?ln=bg" /> <link rel="alternate" hreflang="zh-TW" href="https://cds.cern.ch/record/2636310?ln=zh_TW" /> <link rel="alternate" hreflang="pt" href="https://cds.cern.ch/record/2636310?ln=pt" /> <link rel="alternate" hreflang="no" href="https://cds.cern.ch/record/2636310?ln=no" /> <link rel="alternate" hreflang="hr" href="https://cds.cern.ch/record/2636310?ln=hr" /> <link rel="alternate" hreflang="ca" href="https://cds.cern.ch/record/2636310?ln=ca" /> <link rel="alternate" hreflang="de" href="https://cds.cern.ch/record/2636310?ln=de" /> <link rel="alternate" hreflang="it" href="https://cds.cern.ch/record/2636310?ln=it" /> <link rel="alternate" hreflang="zh-CN" href="https://cds.cern.ch/record/2636310?ln=zh_CN" /> <link rel="alternate" hreflang="sv" href="https://cds.cern.ch/record/2636310?ln=sv" /> <link rel="alternate" hreflang="sk" href="https://cds.cern.ch/record/2636310?ln=sk" /> <link rel="alternate" hreflang="en" href="https://cds.cern.ch/record/2636310?ln=en" /> <link rel="alternate" hreflang="pl" href="https://cds.cern.ch/record/2636310?ln=pl" /> <link rel="alternate" hreflang="ru" href="https://cds.cern.ch/record/2636310?ln=ru" /> <link rel="alternate" hreflang="ka" href="https://cds.cern.ch/record/2636310?ln=ka" /> <link rel="alternate" hreflang="ja" href="https://cds.cern.ch/record/2636310?ln=ja" /> <link rel="alternate" hreflang="es" href="https://cds.cern.ch/record/2636310?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="The European Space Agency’s Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter ΛCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (θ*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the ΛCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances.Key words: cosmology: observations / cosmology: theory / cosmic background radiation / surveys⋆ Corresponding authors: F. R. Bouchet, bouchet@iap.fr; M. White, mwhite@berkeley.edu The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter LCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (theta_*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the LCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances. Aghanim, N.; Akrami, Y.; Arroja, F.; 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.; Bock, J.J.; Bond, J.R.; Borrill, J.; Bouchet, F.R.; Boulanger, F.; Bucher, M.; Burigana, C.; Butler, R.C.; Calabrese, E.; Cardoso, J.-F.; Carron, J.; Casaponsa, B.; Challinor, A.; Chiang, H.C.; Colombo, L.P.L.; Combet, C.; Contreras, D.; Crill, B.P.; Cuttaia, F.; de Bernardis, P.; de Zotti, G.; Delabrouille, J.; Delouis, J.-M.; Désert, F.-X.; Di Valentino, E.; Dickinson, C.; Diego, J.M.; Donzelli, S.; Doré, O.; Douspis, M.; Ducout, A.; Dupac, X.; Efstathiou, G.; Elsner, F.; Enßlin, T.A.; Eriksen, H.K.; Falgarone, E.; Fantaye, Y.; Fergusson, J.; Fernandez-Cobos, R.; Finelli, F.; Forastieri, F.; Frailis, M.; Franceschi, E.; Frolov, A.; Galeotta, S.; Galli, S.; Ganga, K.; Génova-Santos, R.T.; Gerbino, M.; Ghosh, T.; González-Nuevo, J.; Górski, K.M.; Gratton, S.; Gruppuso, A.; Gudmundsson, J.E.; Hamann, J.; Handley, W.; Hansen, F.K.; Helou, G.; Herranz, D.; Hildebrandt, S.R.; Hivon, E.; Huang, Z.; Jaffe, A.H.; Jones, W.C.; Karakci, A.; Keihänen, E.; Keskitalo, R.; Kiiveri, K.; Kim, J.; Kisner, T.S.; Knox, L.; Krachmalnicoff, N.; Kunz, M.; Kurki-Suonio, H.; Lagache, G.; Lamarre, J.-M.; Langer, M.; Lasenby, A.; Lattanzi, M.; Lawrence, C.R.; Le Jeune, M.; Leahy, J.P.; Lesgourgues, J.; Levrier, F.; Lewis, A.; Liguori, M.; Lilje, P.B.; Lilley, M.; Lindholm, V.; López-Caniego, M.; Lubin, P.M.; Ma, Y.-Z.; Macías-Pérez, J.F.; Maggio, G.; Maino, D.; Mandolesi, N.; Mangilli, A.; Marcos-Caballero, A.; Maris, M.; Martin, P.G.; Martinelli, M.; Martínez-González, E.; Matarrese, S.; Mauri, N.; McEwen, J.D.; Meerburg, P.D.; Meinhold, P.R.; Melchiorri, A.; Mennella, A.; Migliaccio, M.; Millea, M.; Mitra, S.; Miville-Deschênes, M.-A.; Molinari, D.; Moneti, A.; Montier, L.; Morgante, G.; Moss, A.; Mottet, S.; Münchmeyer, M.; Natoli, P.; Nørgaard-Nielsen, H.U.; Oxborrow, C.A.; Pagano, L.; Paoletti, D.; Partridge, B.; Patanchon, G.; Pearson, T.J.; Peel, M.; Peiris, H.V.; Perrotta, F.; Pettorino, V.; Piacentini, F.; Polastri, L.; Polenta, G.; Puget, J.-L.; Rachen, J.P.; Reinecke, M.; Remazeilles, M.; Renault, C.; Renzi, A.; Rocha, G.; Rosset, C.; Roudier, G.; Rubiño-Martín, J.A.; Ruiz-Granados, B.; Salvati, L.; Sandri, M.; Savelainen, M.; Scott, D.; Shellard, E.P.S.; Shiraishi, M.; Sirignano, C.; Sirri, G.; Spencer, L.D.; Sunyaev, R.; Suur-Uski, A.-S.; Tauber, J.A.; Tavagnacco, D.; Tenti, M.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Trombetti, T.; Valiviita, J.; Van Tent, B.; Vibert, L.; Vielva, P.; Villa, F.; Vittorio, N.; Wandelt, B.D.; Wehus, I.K.; White, M.; White, Simon D.M.; 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>  <link rel="stylesheet" href="https://cds.cern.ch/img/webnews.css" type="text/css" />  <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>  <meta content="arXiv : Planck 2018 results. 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<meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/conditional_coadd_TT_EE_TE_lfull.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/triangle_TE_delta100.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/triangle_TE_delta100.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/I-FGs.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/I-FGs.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/sz_spectra.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/sz_spectra.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/pps_legacy.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/pps_legacy.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/params_earlyU.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/params_earlyU.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/moll_temp_v2.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/moll_temp_v2.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/H0_ladder2_cropped.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/H0_ladder2_cropped.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/params_lateU.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/params_lateU.png" /> <meta property="og:image" content="https://cds.cern.ch/record/2636310/files/pk_compilation.png" /> <meta property="og:image:secure_url" content="https://cds.cern.ch/record/2636310/files/pk_compilation.png" /> <meta content="CERN Document Server" property="og:site_name" /> <meta content="arXiv" property="og:description" /> <meta content="The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter LCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (theta_*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the LCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances." property="og:description" /> <meta content="EDP Sciences" property="og:description" /> <meta content="The European Space Agency’s Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter ΛCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (θ*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the ΛCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances.Key words: cosmology: observations / cosmology: theory / cosmic background radiation / surveys⋆ Corresponding authors: F. R. Bouchet, bouchet@iap.fr; M. 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I. Overview and the cosmological legacy of Planck </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/2636310/?ln=ru">Информация </a></li><li class=""><a href="/record/2636310/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">  <abbr class="unapi-id" title="2636310"></abbr> <style type="text/css">  </style> <table class="formatRecordTableFullWidth" > <tr> <td class="formatRecordHeader" style="background-image: url('https://cds.cern.ch/img/journals.jpg');" colspan="2">  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:1807.06205">arXiv:1807.06205</a></td></tr> <tr><td class="formatRecordLabel"> Title </td><td style="padding-left:5px;"><b>Planck 2018 results. I. Overview and the cosmological legacy of Planck</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 194 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=Aghanim%2C%20N.&ln=ru">Aghanim, N.</a> (Orsay, IAS) ; <a href="https://cds.cern.ch/search?f=author&p=Akrami%2C%20Y.&ln=ru">Akrami, Y.</a> (Inst. 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Astrophys., Oslo ; Leiden U.) ; <a href="https://cds.cern.ch/search?f=author&p=Arroja%2C%20F.&ln=ru">Arroja, F.</a> (Lisbon U.) ; <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=Aumont%2C%20J.&ln=ru">Aumont, J.</a> (IRAP, Toulouse) ; <a href="https://cds.cern.ch/search?f=author&p=Baccigalupi%2C%20C.&ln=ru">Baccigalupi, C.</a> (CERN) ; <a href="https://cds.cern.ch/search?f=author&p=Ballardini%2C%20M.&ln=ru">Ballardini, M.</a> (Cape Town U. ; IASF, Bologna) ; <a href="https://cds.cern.ch/search?f=author&p=Banday%2C%20A.J.&ln=ru">Banday, A.J.</a> (IRAP, Toulouse) ; <a href="https://cds.cern.ch/search?f=author&p=Barreiro%2C%20R.B.&ln=ru">Barreiro, R.B.</a> (Cantabria U., Santander) ; <a href="https://cds.cern.ch/search?f=author&p=Bartolo%2C%20N.&ln=ru">Bartolo, N.</a> (INFN, Padua ; Padua U.) ; <a href="https://cds.cern.ch/search?f=author&p=Basak%2C%20S.&ln=ru">Basak, S.</a> (IISER, Trivandrum, Sch. 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Astrophys.) ; <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=Langer%2C%20M.&ln=ru">Langer, M.</a> (Orsay, IAS) ; <a href="https://cds.cern.ch/search?f=author&p=Lasenby%2C%20A.&ln=ru">Lasenby, A.</a> (Cambridge U.) ; <a href="https://cds.cern.ch/search?f=author&p=Lattanzi%2C%20M.&ln=ru">Lattanzi, M.</a> (Ferrara U. ; INFN, Ferrara) ; <a href="https://cds.cern.ch/search?f=author&p=Lawrence%2C%20C.R.&ln=ru">Lawrence, C.R.</a> (Caltech, JPL) ; <a href="https://cds.cern.ch/search?f=author&p=Le%20Jeune%2C%20M.&ln=ru">Le Jeune, M.</a> (APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Leahy%2C%20J.P.&ln=ru">Leahy, J.P.</a> (Jodrell Bank) ; <a href="https://cds.cern.ch/search?f=author&p=Lesgourgues%2C%20J.&ln=ru">Lesgourgues, J.</a> (Aachen, Tech. Hochsch.) ; <a href="https://cds.cern.ch/search?f=author&p=Levrier%2C%20F.&ln=ru">Levrier, F.</a> (LERMA, Ivry) ; <a href="https://cds.cern.ch/search?f=author&p=Lewis%2C%20A.&ln=ru">Lewis, A.</a> (Sussex U.) ; <a href="https://cds.cern.ch/search?f=author&p=Liguori%2C%20M.&ln=ru">Liguori, M.</a> (INFN, Padua ; Padua U.) ; <a href="https://cds.cern.ch/search?f=author&p=Lilje%2C%20P.B.&ln=ru">Lilje, P.B.</a> (Inst. Theor. Astrophys., Oslo) ; <a href="https://cds.cern.ch/search?f=author&p=Lilley%2C%20M.&ln=ru">Lilley, M.</a> (Paris, Inst. 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Theor. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Martinelli%2C%20M.&ln=ru">Martinelli, M.</a> (Heidelberg U.) ; <a href="https://cds.cern.ch/search?f=author&p=Mart%C3%ADnez-Gonz%C3%A1lez%2C%20E.&ln=ru">Martínez-González, E.</a> (Cantabria U., Santander) ; <a href="https://cds.cern.ch/search?f=author&p=Matarrese%2C%20S.&ln=ru">Matarrese, S.</a> (GSSI, Aquila ; INFN, Padua ; Padua U.) ; <a href="https://cds.cern.ch/search?f=author&p=Mauri%2C%20N.&ln=ru">Mauri, N.</a> (INFN, Bologna ; U. Bologna, DIFA) ; <a href="https://cds.cern.ch/search?f=author&p=McEwen%2C%20J.D.&ln=ru">McEwen, J.D.</a> (Mullard Space Sci. 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Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=M%C3%BCnchmeyer%2C%20M.&ln=ru">Münchmeyer, M.</a> (Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Natoli%2C%20P.&ln=ru">Natoli, P.</a> (Ferrara U. ; INFN, Ferrara) ; <a href="https://cds.cern.ch/search?f=author&p=N%C3%B8rgaard-Nielsen%2C%20H.U.&ln=ru">Nørgaard-Nielsen, H.U.</a> (Denmark, Tech. U.) ; <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=Pagano%2C%20L.&ln=ru">Pagano, L.</a> (LERMA, Ivry ; Orsay, IAS) ; <a href="https://cds.cern.ch/search?f=author&p=Paoletti%2C%20D.&ln=ru">Paoletti, D.</a> (IASF, Bologna ; INFN, Bologna) ; <a href="https://cds.cern.ch/search?f=author&p=Partridge%2C%20B.&ln=ru">Partridge, B.</a> (Haverford Coll.) ; <a href="https://cds.cern.ch/search?f=author&p=Patanchon%2C%20G.&ln=ru">Patanchon, G.</a> (APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Pearson%2C%20T.J.&ln=ru">Pearson, T.J.</a> (Caltech) ; <a href="https://cds.cern.ch/search?f=author&p=Peel%2C%20M.&ln=ru">Peel, M.</a> (Jodrell Bank ; Sao Paulo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Peiris%2C%20H.V.&ln=ru">Peiris, H.V.</a> (University Coll. London) ; <a href="https://cds.cern.ch/search?f=author&p=Perrotta%2C%20F.&ln=ru">Perrotta, F.</a> (INFN, Trieste ; SISSA, Trieste) ; <a href="https://cds.cern.ch/search?f=author&p=Pettorino%2C%20V.&ln=ru">Pettorino, V.</a> (AIM, Saclay) ; <a href="https://cds.cern.ch/search?f=author&p=Piacentini%2C%20F.&ln=ru">Piacentini, F.</a> (Rome U.) ; <a href="https://cds.cern.ch/search?f=author&p=Polastri%2C%20L.&ln=ru">Polastri, L.</a> (Ferrara U. ; INFN, Ferrara) ; <a href="https://cds.cern.ch/search?f=author&p=Polenta%2C%20G.&ln=ru">Polenta, G.</a> (ASI, Rome) ; <a href="https://cds.cern.ch/search?f=author&p=Puget%2C%20J.-L.&ln=ru">Puget, J.-L.</a> (Orsay, IAS) ; <a href="https://cds.cern.ch/search?f=author&p=Rachen%2C%20J.P.&ln=ru">Rachen, J.P.</a> (Nijmegen U., IMAPP) ; <a href="https://cds.cern.ch/search?f=author&p=Reinecke%2C%20M.&ln=ru">Reinecke, M.</a> (Garching, Max Planck Inst., MPE) ; <a href="https://cds.cern.ch/search?f=author&p=Remazeilles%2C%20M.&ln=ru">Remazeilles, M.</a> (Jodrell Bank) ; <a href="https://cds.cern.ch/search?f=author&p=Renault%2C%20C.&ln=ru">Renault, C.</a> (LPSC, Grenoble) ; <a href="https://cds.cern.ch/search?f=author&p=Renzi%2C%20A.&ln=ru">Renzi, A.</a> (INFN, Padua) ; <a href="https://cds.cern.ch/search?f=author&p=Rocha%2C%20G.&ln=ru">Rocha, G.</a> (Caltech ; Caltech, JPL) ; <a href="https://cds.cern.ch/search?f=author&p=Rosset%2C%20C.&ln=ru">Rosset, C.</a> (APC, Paris) ; <a href="https://cds.cern.ch/search?f=author&p=Roudier%2C%20G.&ln=ru">Roudier, G.</a> (APC, Paris ; Caltech, JPL ; LERMA, Ivry) ; <a href="https://cds.cern.ch/search?f=author&p=Rubi%C3%B1o-Mart%C3%ADn%2C%20J.A.&ln=ru">Rubiño-Martín, J.A.</a> (IAC, La Laguna ; Laguna U., Tenerife) ; <a href="https://cds.cern.ch/search?f=author&p=Ruiz-Granados%2C%20B.&ln=ru">Ruiz-Granados, B.</a> (IAC, La Laguna ; Laguna U., Tenerife) ; <a href="https://cds.cern.ch/search?f=author&p=Salvati%2C%20L.&ln=ru">Salvati, L.</a> (Orsay, IAS) ; <a href="https://cds.cern.ch/search?f=author&p=Sandri%2C%20M.&ln=ru">Sandri, M.</a> (IASF, Bologna) ; <a href="https://cds.cern.ch/search?f=author&p=Savelainen%2C%20M.&ln=ru">Savelainen, M.</a> (Aalto U. ; Helsinki Inst. of Phys. ; Helsinki U.) ; <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=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=Shiraishi%2C%20M.&ln=ru">Shiraishi, M.</a> (INFN, Padua ; Kagawa U. ; Padua U.) ; <a href="https://cds.cern.ch/search?f=author&p=Sirignano%2C%20C.&ln=ru">Sirignano, C.</a> (INFN, Padua ; Padua U.) ; <a href="https://cds.cern.ch/search?f=author&p=Sirri%2C%20G.&ln=ru">Sirri, G.</a> (INFN, Bologna ; U. Bologna, DIFA) ; <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=Sunyaev%2C%20R.&ln=ru">Sunyaev, R.</a> (Garching, Max Planck Inst., MPE ; Moscow, Space Res. Inst.) ; <a href="https://cds.cern.ch/search?f=author&p=Suur-Uski%2C%20A.-S.&ln=ru">Suur-Uski, A.-S.</a> (Helsinki Inst. of Phys. ; Helsinki U.) ; <a href="https://cds.cern.ch/search?f=author&p=Tauber%2C%20J.A.&ln=ru">Tauber, J.A.</a> (ESTEC, Noordwijk) ; <a href="https://cds.cern.ch/search?f=author&p=Tavagnacco%2C%20D.&ln=ru">Tavagnacco, D.</a> (Trieste Observ. ; Trieste U.) ; <a href="https://cds.cern.ch/search?f=author&p=Tenti%2C%20M.&ln=ru">Tenti, M.</a> (INFN, Bologna ; U. Bologna, DIFA) ; <a href="https://cds.cern.ch/search?f=author&p=Terenzi%2C%20L.&ln=ru">Terenzi, L.</a> (IASF, Bologna) ; <a href="https://cds.cern.ch/search?f=author&p=Toffolatti%2C%20L.&ln=ru">Toffolatti, L.</a> (IASF, Bologna ; Oviedo U.) ; <a href="https://cds.cern.ch/search?f=author&p=Tomasi%2C%20M.&ln=ru">Tomasi, M.</a> (IASF, Milan ; Milan U.) ; <a href="https://cds.cern.ch/search?f=author&p=Trombetti%2C%20T.&ln=ru">Trombetti, T.</a> (INAF-IRA, Bologna ; INFN, Ferrara) ; <a href="https://cds.cern.ch/search?f=author&p=Valiviita%2C%20J.&ln=ru">Valiviita, J.</a> (Helsinki Inst. of Phys. ; Helsinki U.) ; <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=Vibert%2C%20L.&ln=ru">Vibert, L.</a> (Orsay, IAS ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Vielva%2C%20P.&ln=ru">Vielva, P.</a> (Cantabria U., Santander) ; <a href="https://cds.cern.ch/search?f=author&p=Villa%2C%20F.&ln=ru">Villa, F.</a> (Frascati) ; <a href="https://cds.cern.ch/search?f=author&p=Vittorio%2C%20N.&ln=ru">Vittorio, N.</a> (Rome U., Tor Vergata) ; <a href="https://cds.cern.ch/search?f=author&p=Wandelt%2C%20B.D.&ln=ru">Wandelt, B.D.</a> (Illinois U., Urbana ; Paris, Inst. Astrophys.) ; <a href="https://cds.cern.ch/search?f=author&p=Wehus%2C%20I.K.&ln=ru">Wehus, I.K.</a> (Caltech, JPL ; Inst. Theor. Astrophys., Oslo) ; <a href="https://cds.cern.ch/search?f=author&p=White%2C%20M.&ln=ru">White, M.</a> (LBL, Berkeley ; UC, Berkeley) ; <a href="https://cds.cern.ch/search?f=author&p=White%2C%20Simon%20D.M.&ln=ru">White, Simon D.M.</a> (Garching, Max Planck Inst., MPE) ; <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> (San Diego, CASS)</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;">2020-09-01</td></tr> <tr><td class="formatRecordLabel"> Imprint </td><td style="padding-left:5px;">2018-07-17</td></tr> <tr><td class="formatRecordLabel"> Number of pages </td><td style="padding-left:5px;">56</td></tr> <tr><td class="formatRecordLabel"> Note </td><td style="padding-left:5px;">61 pages, 40 figures, matches version accepted by A&A</td></tr> <tr><td class="formatRecordLabel"> In: </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1051/0004-6361/201833880"><i>Astron. Astrophys.</i> 641 (2020) A1</a> </a></td></tr> <tr><td class="formatRecordLabel"> DOI </td><td style="padding-left:5px;"><a href="http://dx.doi.org/10.1051/0004-6361/201833880" title="DOI" target="_blank">10.1051/0004-6361/201833880</a> (publication) <tr><td class="formatRecordLabel"> Subject category </td><td style="padding-left:5px;">astro-ph.CO ; 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&f=693__e">PLANCK</a></td></tr> <tr><td class="formatRecordLabel"> Abstract </td><td style="padding-left:5px;">The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter LCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (theta_*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the LCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances.</td></tr> <tr><td class="formatRecordLabel"> Copyright/License </td><td style="padding-left:5px;">preprint: (License: <a href="http://arxiv.org/licenses/nonexclusive-distrib/1.0/">arXiv nonexclusive-distrib 1.0</a>)</td></tr> </table> <br /><div style="max-width:1024px;margin:auto"><div style="overflow-x:auto;display:inline;width:100%;"><a href="/record/2636310/plots#0"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2636310/files/2018_T_9_FREQ_v1_rotated.png" title=" Fluctuations of the sky emission in each of the nine \Planck\ frequency bands, after removal of a common dipole component. The fluctuations are expressed as equivalent temperature variations at each of the seven lowest frequencies, so that fluctuations with a thermal spectrum will appear the same in each map (except for the effects of the varying resolution of the maps). The highest frequencies, which monitor the dust emission, are expressed in more conventional units." width="200px"/></a> <a href="/record/2636310/plots#0"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2636310/files/2018_T_9_FREQ_v3_rotated.png" title=" Fluctuations of sky emission in each of nine \Planck\ frequency bands, after removal of a common dipole component. The fluctuations are expressed as equivalent temperature variations at each of the seven lowest frequencies, so that fluctuations with a thermal spectrum will appear the same in each map (except for the effects of the varying resolution of the maps). The highest frequencies, which monitor the dust emission, are expressed in more conventional units." width="200px"/></a> <a href="/record/2636310/plots#1"><img style="vertical-align:middle;" src="https://cds.cern.ch/record/2636310/files/2018_QUP.png" title=" Sky polarization in seven polarized frequency bands of \Planck. The first two columns show the $Q$ and $U$ Stokes parameters; the last column indicates the polarized intensity, $P=\sqrt{Q^2+U^2}$ (although this emphasizes the strength of polarization in noisy regions). In addition to the rich science that they enable on their own, these maps set the baseline for all future CMB polarization experiments, for example by defining the most cosmologically challenged areas." width="200px"/></a> <a href='/record/2636310/plots'>Show more plots</a></div></div><br /> <br/>Corresponding record in: <a href="http://inspirehep.net/record/1682875">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 2018-08-28, последняя модификация 2024-10-16</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%3A2636310&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 /><em>1807.06205</em> - <a href="/record/2636310/files/1807.06205.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="Загрузка полного текста"/>PDF</a><br /><em>arXiv:1807.06205</em> - <a href="/record/2636310/files/arXiv:1807.06205.pdf"><img style="border:none" src="/img/file-icon-text-12x16.gif" alt="Загрузка полного текста"/>PDF</a><br /></div> </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=2636310">Добавить в личную книжную полку</a></li> <li>Экспортировать как <a style="text-decoration:underline;font-weight:normal" href="/record/2636310/export/hx?ln=ru">BibTeX</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2636310/export/hm?ln=ru">MARC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2636310/export/xm?ln=ru">MARCXML</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2636310/export/xd?ln=ru">DC</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2636310/export/xe?ln=ru">EndNote</a>,  <a style="text-decoration:underline;font-weight:normal" href="/record/2636310/export/xn?ln=ru">NLM</a>, <a style="text-decoration:underline;font-weight:normal" href="/record/2636310/export/xw?ln=ru">RefWorks</a> </li> </ul> <div style='padding-left: 13px;'>  <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/1807.0620/add'); $('#bookmark_sciencewise').bookmark({sites: ['sciencewise']}); $('#bookmark').bookmark({ sites: ['facebook', 'twitter', 'linkedin', 'google_plusone'], icons: '/img/bookmarks.png', url: 'https://cds.cern.ch/record/2636310', addEmail: true, title: "Planck 2018 results. I. Overview and the cosmological legacy of Planck", description: "The European Space Agency\u2019s Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter \u039bCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (\u03b8*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the \u039bCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances.Key words: cosmology: observations / cosmology: theory / cosmic background radiation / surveys\u22c6 Corresponding authors: F. R. Bouchet, bouchet@iap.fr; M. 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