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CERN Document Server 2,041 ჩანაწერია ნაპოვნი  1 - 10შემდეგიდასასრული  ჩანაწერთან გადასვლა: ძიებას დასჭირდა 1.03 წამი. 
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Planck 2013 results. XIII. Galactic CO emission / Planck collaboration
Rotational transition lines of CO play a major role in molecular radio astronomy and in particular in the study of star formation and the Galactic structure. Although a wealth of data exists in the Galactic plane and some well-known molecular clouds, there is no available CO high sensitivity all-sky survey to date. [...]
arXiv:1303.5073; CERN-PH-TH-2013-126; CERN-PH-TH-2013-126.- 2014-10-29 - 22 p. - Published in : Astron. Astrophys. 571 (2014) A13 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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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
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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Planck 2013 results. XII. Diffuse component separation / Planck Collaboration
Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwave background (CMB) temperature fluctuations over nearly the full sky, as well as new constraints on Galactic foregrounds. [...]
arXiv:1303.5072; CERN-PH-TH-2013-125; CERN-PH-TH-2013-125.- 2014-10-29 - 31 p. - Published in : Astron. Astrophys. 571 (2014) A12 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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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
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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Planck 2013 results. VIII. HFI photometric calibration and mapmaking / Planck Collaboration
This paper describes the processing applied to the HFI cleaned time-ordered data to produce photometrically calibrated maps. HFI observes the sky over a broad range of frequencies, from 100 to 857 GHz. [...]
arXiv:1303.5069; CERN-PH-TH-2013-122; CERN-PH-TH-2013-122.- 2014-10-29 - 25 p. - Published in : Astron. Astrophys. 571 (2014) A8 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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Planck 2013 results. IX. HFI spectral response / Planck Collaboration
The Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground based tests conducted with the HFI focal plane in a cryogenic environment prior to launch. The main goal of the spectral transmission tests was to measure the relative spectral response (including out-of-band signal rejection) of all HFI detectors. [...]
arXiv:1303.5070; CERN-PH-TH-2013-123; CERN-PH-TH-2013-123.- 2014-10-29 - 27 p. - Published in : Astron. Astrophys. 571 (2014) A9 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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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
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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Planck 2013 results. VII. HFI time response and beams / Planck Collaboration
This paper characterizes the effective beams,the effective beam window functions and the associated errors for the Planck HFI detectors. The effective beam is the angular response including the effect of the optics,detectors,data processing and the scan strategy. [...]
arXiv:1303.5068; CERN-PH-TH-2013-121; CERN-PH-TH-2013-121.- 2014-10-29 - 31 p. - Published in : Astron. Astrophys. 571 (2014) A7 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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Planck 2013 results. III. LFI systematic uncertainties / Planck Collaboration
We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. [...]
arXiv:1303.5064; CERN-PH-TH-2013-117; CERN-PH-TH-2013-117.- 2014-10-29 - 23 p. - Published in : Astron. Astrophys. 571 (2014) A3 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article
დეტალური ჩანაწერი - მსგავსი ჩანაწერები
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Fine structure in the α decay of At218 / IS534 Collaboration
2019 - Published in : 10.1103/PhysRevC.99.064317
დეტალური ჩანაწერი - მსგავსი ჩანაწერები

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