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CERN Document Server 找到 9 笔记录  检索需时 0.62 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. [...]
arXiv:2405.13491. - 94.
Fulltext
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2.
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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3.
Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps / Planck Collaboration
This paper describes the processing applied to the Planck High Frequency Instrument (HFI) cleaned, time-ordered information to produce photometrically calibrated maps in temperature and (for the first time) in polarization. The data from the 2.5 year full mission include almost five independent full-sky surveys. [...]
arXiv:1502.01587.- 2016-09-20 - 27 p. - Published in : Astron. Astrophys. 594 (2016) A8 Fulltext: PDF; External link: Preprint
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4.
Planck 2015 results. VII. HFI TOI and beam processing / Planck Collaboration
The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polarization (100, 143, 217, and 353 GHz). In order to obtain sky maps, the time-ordered information (TOI) containing the detector and pointing samples must be processed and the angular response must be assessed. [...]
arXiv:1502.01586.- 2016-09-20 - 30 p. - Published in : Astron. Astrophys. 594 (2016) A7 Fulltext: PDF; External link: Preprint
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5.
Planck 2015 results. I. Overview of products and scientific results / Planck Collaboration
The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October 2013. In February~2015, ESA and the Planck Collaboration released the second set of cosmology products based on data from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. [...]
arXiv:1502.01582.- 2016-09-20 - 38 p. - Published in : Astron. Astrophys. 594 (2016) A1 Fulltext: PDF; External link: Preprint
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6.
Planck 2013 results. XIV. Zodiacal emission / Planck Collaboration
The Planck satellite provides a set of all-sky maps at nine frequencies from 30 GHz to 857 GHz. Planets, minor bodies, and diffuse interplanetary dust emission (IPD) are all observed. [...]
arXiv:1303.5074; CERN-PH-TH-2013-127; CERN-PH-TH-2013-127.- 2014-10-29 - 25 p. - Published in : Astron. Astrophys. 571 (2014) A14 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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7.
Planck 2013 results X. Energetic particle effects: characterization, removal, and simulation / Planck Collaboration
This paper presents the detection, interpretation and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI). These interactions fall into two categories, heating the 0.1 K bolometer plate and glitches in each detector time stream. [...]
arXiv:1303.5071; CERN-PH-TH-2013-124; CERN-PH-TH-2013-124.- 2014-10-29 - 23 p. - Published in : Astron. Astrophys. 571 (2014) A10 Fulltext: arXiv:1303.5071 - PDF; 1303.5071 - PDF; External links: Preprint; EDP Sciences Free Access article
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8.
Planck 2013 results. VI. High Frequency Instrument data processing / Planck Collaboration
We describe the processing of the 531 billion raw data samples from the High Frequency Instrument (hereafter HFI), which we performed to produce six temperature maps from the first 473 days of Planck-HFI survey data. These maps provide an accurate rendition of the sky emission at 100, 143, 217, 353, 545, and 857 GHz with an angular resolution ranging from 9.7 to 4.6 arcmin. [...]
arXiv:1303.5067; CERN-PH-TH-2013-120; CERN-PH-TH-2013-120.- 2014-10-29 - 44 p. - Published in : Astron. Astrophys. 571 (2014) A6 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
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9.
The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths / Delabrouille, J. (APC, Paris) ; Betoule, M. ; Melin, J.-B. ; Miville-Deschenes, M.-A. ; Gonzalez-Nuevo, J. ; Jeune, M.Le (APC, Paris) ; Castex, G. ; de Zotti, G. ; Basak, S. (APC, Paris) ; Ashdown, M. et al.
We present the Planck Sky Model (PSM), a parametric model for the generation of all-sky, few arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, in both intensity and polarisation. Several options are implemented to model the cosmic microwave background, Galactic diffuse emission (synchrotron, free-free, thermal and spinning dust, CO lines), Galactic H-II regions, extragalactic radio sources, dusty galaxies, and thermal and kinetic Sunyaev-Zeldovich signals from clusters of galaxies. [...]
arXiv:1207.3675.- 2012 - 35 p. - Published in : Astron. Astrophys. 553 (2013) A96 External link: Preprint
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1 Mottet, S
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