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CERN Document Server 找到 2,047 筆記錄  1 - 10下一個最後  跳到記錄: 檢索需時 2.36 秒. 
1.
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Science with the Cherenkov Telescope Array / Cherenkov Telescope Array Consortium Collaboration
The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. [...]
arXiv:1709.07997. - 2017. - 211 p.
Preprint
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2.
(91)
Euclid Definition Study Report / Laureijs, R. (ESTEC, Noordwijk) ; Amiaux, J. (DAPNIA, Saclay) ; Arduini, S. (Paris U., VI-VII) ; Augueres, J.L. (DAPNIA, Saclay) ; Brinchmann, J. (Leiden U.) ; Cole, R. (University Coll. London) ; Cropper, M. (University Coll. London) ; Dabin, C. (CNES, Toulouse) ; Duvet, L. (ESTEC, Noordwijk) ; Ealet, A. (Marseille, CPPM) et al.
Euclid is a space-based survey mission from the European Space Agency designed to understand the origin of the Universe's accelerating expansion. [...]
arXiv:1110.3193 ; ESA-SRE(2011)12 ; ESA-SRE(2011)12. - 2011. - 116 p.
Preprint - Full text
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Planck 2018 results. I. Overview and the cosmological legacy of Planck / Planck Collaboration
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. [...]
arXiv:1807.06205.- 2020-09-01 - 56 p. - Published in : Astron. Astrophys. 641 (2020) A1 Fulltext: 1807.06205 - PDF; arXiv:1807.06205 - PDF;
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4.
(78)
The AGILE Mission / AGILE Collaboration
AGILE is an Italian Space Agency mission dedicated to the observation of the gamma-ray Universe. The AGILE very innovative instrumentation combines for the first time a gamma-ray imager (sensitive in the energy range 30 MeV - 50 GeV), a hard X-ray imager (sensitive in the range 18-60 keV) together with a Calorimeter (sensitive in the range 300 keV - 100 MeV) and an anticoincidence system. [...]
arXiv:0807.4254.- 2008 - 20 p. - Published in : Astron. Astrophys. 502 (2009) 995-1013 Preprint: PDF; External link: Preprint
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5.
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Planck 2015 results. V. LFI calibration / Planck Collaboration
We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the CMB dipole, exploiting both the orbital and solar components. [...]
arXiv:1505.08022.- 2016-09-20 - 24 p. - Published in : Astron. Astrophys. 594 (2016) A5 Fulltext: PDF; External link: Preprint
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Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources / Planck Collaboration
We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev--Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. The catalogue contains 1227 entries, making it over six times the size of the Planck Early SZ (ESZ) sample and the largest SZ-selected catalogue to date. [...]
arXiv:1303.5089; CERN-PH-TH-2013-141; CERN-PH-TH-2013-141.- 2014-10-29 - 41 p. - Published in : Astron. Astrophys. 571 (2014) A29 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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Planck 2013 results. XV. CMB power spectra and likelihood / Planck collaboration
We present the Planck likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations. We use this likelihood to derive the Planck CMB power spectrum over three decades in l, covering 2 <= l <= 2500 [...]
arXiv:1303.5075; CERN-PH-TH-2013-128; CERN-PH-TH-2013-128.- 2014-10-29 - 60 p. - Published in : Astron. Astrophys. 571 (2014) A15 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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8.
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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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Planck 2013 results. XVI. Cosmological parameters / Planck Collaboration
We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. [...]
arXiv:1303.5076; CERN-PH-TH-2013-129; CERN-PH-TH-2013-129.- 2014-10-29 - 66 p. - Published in : Astron. Astrophys. 571 (2014) A16 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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Planck 2015 results. XVI. Isotropy and statistics of the CMB / Planck Collaboration
We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly on the full Planck mission for temperature, but also include some polarization measurements. [...]
arXiv:1506.07135.- 2016-09-20 - 62 p. - Published in : Astron. Astrophys. 594 (2016) A16 Fulltext: PDF; External link: Preprint
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