Search results

Create the page "Planckpapers" on this wiki! See also the search results found.

• HFI design, qualification, and performance
  ...detail this information are available: {{PlanckPapers|lamarre2010}} and {{PlanckPapers|planck2011-1-5}}. Additional detailed information potentially useful for th
  5 KB (778 words) - 15:28, 22 July 2014
• LFI design, qualification, and performance
  ...can be written as follows{{BibCite|seiffert2002}}{{BibCite|mennella2003}}{{PlanckPapers|bersanelli2010}}:: The gain modulation factor{{BibCite|mennella2003}}{{PlanckPapers|planck2011-1-6}}, <math>r</math>, is defined by:
  50 KB (7,790 words) - 10:04, 23 July 2014
• The HFI DPC
  ...es of publications was described in {{PlanckPapers|planck2011-1-7}}. The {{PlanckPapers|planck2013-p03}} and its co-papers provide the reference for the processin ...other R&D groups in the HFI and LFI core teams. An overview was given in {{PlanckPapers|planck2011-1-7}}. In particular:
  4 KB (619 words) - 13:50, 23 July 2014
• The LFI DPC
  ...nckPapers|planck2013-p02b}}, and instrument performances are reported in {{PlanckPapers|planck2013-p02a}}.
  7 KB (1,004 words) - 15:06, 23 July 2014
• Simulation data
  ...t decorrelation observed in the Planck Early Paper on CIB power spectrum {{PlanckPapers|planck2011-6-6}}. ...haracterisation of this lensing potential map are described in detail in {{PlanckPapers|planck2013-p12}}, which describes also the procedure used to generate the r
  28 KB (4,118 words) - 16:15, 15 October 2015
• Specially processed maps
  ...e (MV) lens reconstruction which forms the basis for the main results of {{PlanckPapers|planck2013-p12}}. This map is produced using a combination of the 143 and 2 ...spectrum on the local noise level of the map, discussed in Appendix A of {{PlanckPapers|planck2013-p12}}. Note that the noise power spectrum estimate here is not s
  7 KB (921 words) - 17:34, 23 July 2014
• Catalogues
  # The Planck beams are described in {{PlanckPapers|planck2013-p02d}} and {{PlanckPapers|planck2013-p03c}}. This table shows the values which were adopted for the P # In the extragalactic zone (48% of the sky; see Fig. 2 in {{PlanckPapers|planck2013-p05}}).
  30 KB (4,218 words) - 16:56, 23 July 2014
• CMB spectrum & Likelihood Code
  .../math>, instead, the spectrum is derived from the ''CAMspec'' likelihood {{PlanckPapers|planck2013-p08}} by optimally combining the spectra in the frequency range ...nck best-fit primordial power spectrum (cf Planck+WP+highL in Table 5 of {{PlanckPapers|planck2013-p11}}).''']]
  17 KB (2,601 words) - 17:28, 23 July 2014
• Pre-processing
  ...ience data is retrieved and reconstructed as described in section 3.1 of {{PlanckPapers|planck2011-1-7|5}}. ...using a spherical linear interpolation as described in section 3.4 of of {{PlanckPapers|planck2011-1-7|6}}.
  13 KB (1,976 words) - 13:53, 23 July 2014
• Sky temperature maps
  ...sting them to astrophysical values is given in the HFI Calibration paper {{PlanckPapers|planck2013-p03b}}. ...vel monopole by applying an offset correction, see LFI Calibration paper {{PlanckPapers|planck2013-p02b}} section 3.4 "Setting the zero levels in the maps". Note t
  35 KB (5,220 words) - 13:00, 24 July 2014
• Map-making
  ...nd its performances are described in {{PlanckPapers|planck2013-p03}} and {{PlanckPapers|planck2013-p03b}}. ...on is removed from the 353, 545 and 857 GHz channels. It is described in {{PlanckPapers|planck2013-p03}}, but a synopsis of the procedure is as follows:
  11 KB (1,710 words) - 14:31, 23 July 2014
• The RIMO
  ...passes of the detectors that are used to build the map. For details see {{PlanckPapers|planck2013-p03d}}. The bandpasses are given as 4-column tables containing: ...ssist in CO component separation efforts {{PlanckPapers|planck2013-p03a}}{{PlanckPapers|planck2013-p03d}}.
  12 KB (1,821 words) - 16:42, 23 July 2014
• TOI processing
  ...tures of the pipeline which are given in the HFI Data Processing article {{PlanckPapers|planck2013-p03}}. Here we give complementary explanations on some details. ...glitch rate per channel is shown in this figure. For details, see copap. {{PlanckPapers|planck2013-p03e}}.
  18 KB (2,712 words) - 13:55, 23 July 2014
• The Planck mission
  For more information, see {{PlanckPapers|planck2011-1-1}}. For a complete list of operational events, including cont More details on the Planck mission performance can be found in {{PlanckPapers|planck2011-1-1}}.
  16 KB (2,489 words) - 13:19, 22 July 2014
• Ground Segment and Operations
  More information about the Planck Ground Segment may be found in {{PlanckPapers|tauber2010a}}.
  4 KB (601 words) - 14:24, 22 July 2014
• TOI processing LFI
  ...ogic/Digital Converter on board. More on {{PlanckPapers|planck2013-p02}},{{PlanckPapers|planck2013-p02a}}. ...lines. More information can be found in {{PlanckPapers|planck2013-p02}}, {{PlanckPapers|planck2013-p02a}}.
  31 KB (4,941 words) - 15:14, 23 July 2014
• HFI cryogenics
  ...constant. The dilution cooler is described in detail in section 2.3.3 of {{PlanckPapers|planck2011-1-3|7}}. 5.4 of {{PlanckPapers|planck2011-1-3|23}}.
  5 KB (747 words) - 15:36, 22 July 2014
• HFI-Validation
  ...tics]] and in [[#Cosmic_Rays|the section on cosmic rays]], as well as in {{PlanckPapers|planck2013-p03e|1|the 2013 HFI Cosmic Ray Removal paper}}. ...y specific frequency signatures, which is filtered. This is described in {{PlanckPapers|planck2013-p03|1|the 2013 HFI DPC Paper}}, [[#4K_lines_Residuals|the sectio
  25 KB (4,008 words) - 15:01, 23 July 2014
• Map-making LFI
  A detailed description of the map-making procedure is given in {{PlanckPapers|planck2013-p02}}. See also section [[Frequency Maps]]. ...}. We chose to downgrade the maps using the inverse noise weighting. See {{PlanckPapers|planck2013-p02}} for discussion.
  23 KB (3,368 words) - 15:56, 23 July 2014
• Beams LFI
  ...fit as in {{PlanckPapers|planck2011-1-6}} with modification explained in {{PlanckPapers|planck2013-p02d}}. This method is used to determine ...cs code) by appropriately tuning the Radio Frequency Flight Model (RFFM) {{PlanckPapers|tauber2010b}}. The Radio Frequency Tuned Model, called RFTM, was implemente
  23 KB (3,650 words) - 15:53, 23 July 2014

View (previous 20 | next 20) (20 | 50 | 100 | 250 | 500)