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CERN Document Server 找到 6 笔记录  检索需时 0.78 秒. 
1.
Euclid. I. Overview of the Euclid mission / Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14,000 deg^2 of extragalactic sky. [...]
arXiv:2405.13491.- 2025-04 - 94 p. - Published in : Astron. Astrophys. 697 (2025) A1 Fulltext: 2405.13491 - PDF; publication - PDF;
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2.
CMB-S4: Forecasting Constraints on Primordial Gravitational Waves / CMB-S4 Collaboration
CMB-S4---the next-generation ground-based cosmic microwave background (CMB) experiment---is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the Universe, from the highest energies at the dawn of time through the growth of structure to the present day. [...]
arXiv:2008.12619 ; FERMILAB-PUB-20-468-AE-SCD. - 24 p.
Fulltext - Fulltext
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3.
Updated design of the CMB polarization experiment satellite LiteBIRD / Sugai, H. (Tokyo U., IPMU) ; Ade, P.A.R. (Cardiff U.) ; Akiba, Y. (KEK, Tsukuba ; Sokendai, Tsukuba) ; Alonso, D. (Oxford U.) ; Arnold, K. (UC, San Diego) ; Aumont, J. (IRAP, Toulouse) ; Austermann, J. (NIST, Boulder) ; Baccigalupi, C. (CNR, Italy ; INFN, Trieste ; SISSA, Trieste) ; Banday, A.J. (IRAP, Toulouse) ; Banerji, R. (Oslo U.) et al.
Recent developments of transition-edge sensors (TESs), based on extensive experience in ground-based experiments, have been making the sensor techniques mature enough for their application on future satellite CMB polarization experiments. LiteBIRD is in the most advanced phase among such future satellites, targeting its launch in Japanese Fiscal Year 2027 (2027FY) with JAXA's H3 rocket. [...]
arXiv:2001.01724.- 2020-01-27 - 11 p. - Published in : J. Low Temp. Phys. 199 (2020) 1107-1117 Fulltext: s10909-019-02329-w - PDF; 2001.01724 - PDF;
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4.
Exploring cosmic origins with CORE: Survey requirements and mission design / CORE Collaboration
Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. [...]
arXiv:1706.04516.- 2018-04-05 - 79 p. - Published in : JCAP Fulltext: PDF; Preprint: PDF;
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5.
Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts / Planck Collaboration
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. [...]
arXiv:1303.5080; CERN-PH-TH-2013-133; CERN-PH-TH-2013-133.- 2014-10-29 - 20 p. - Published in : Astron. Astrophys. 571 (2014) A20 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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6.
Planck 2013 results. I. Overview of products and scientific results / Planck Collaboration
The ESA's Planck satellite, dedicated to studying the early universe, was launched on May 2009 and has been surveying the microwave and submillimetre sky since August 2009. In March 2013, ESA and the Planck Collaboration publicly released the initial cosmology products based on the first 15.5 months of Planck operations, along with a set of scientific and technical papers and a web-based explanatory supplement. [...]
arXiv:1303.5062; CERN-PH-TH-2013-115; CERN-PH-TH-2013-115.- 2014-10-29 - 48 p. - Published in : Astron. Astrophys. 571 (2014) A1 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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