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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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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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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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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

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ISO observations of Mars : an estimate of the water vapor vertical distribution and the surface emissivity / Burgdorf, M J ; Encrenaz, T ; Lellouch, E ; Feuchtgruber, H ; Davis, G ; Swinyard, B ; De Graauw, T ; Morris, P ; Sidher, S D ; Griffin, M et al.
ESLAB-1999-013-ISO. - 1999. - 34 p.
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Se också: liknande författarnamn
47	Lellouch, E
7	Lellouch, Emmanuel

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