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- ...detail this information are available: {{PlanckPapers|lamarre2010}} and {{PlanckPapers|planck2011-1-5}}. Additional detailed information potentially useful for th5 KB (778 words) - 15:28, 22 July 2014
- ...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
- ...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
- ...nckPapers|planck2013-p02b}}, and instrument performances are reported in {{PlanckPapers|planck2013-p02a}}.7 KB (1,004 words) - 15:06, 23 July 2014
- ...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 r28 KB (4,118 words) - 16:15, 15 October 2015
- ...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 s7 KB (921 words) - 17:34, 23 July 2014
- # 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
- .../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
- ...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
- ...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 t35 KB (5,220 words) - 13:00, 24 July 2014
- ...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
- ...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
- ...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
- 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
- More information about the Planck Ground Segment may be found in {{PlanckPapers|tauber2010a}}.4 KB (601 words) - 14:24, 22 July 2014
- ...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
- ...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
- ...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 sectio25 KB (4,008 words) - 15:01, 23 July 2014
- 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
- ...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 implemente23 KB (3,650 words) - 15:53, 23 July 2014
- All the details can be found in {{PlanckPapers|planck2013-p02}}.13 KB (1,992 words) - 16:09, 23 July 2014
- The cold optics is described in {{PlanckPapers|ade2010}}}. ...description of the HFI optical design and beam performances is given in {{PlanckPapers|maffei2010}}.25 KB (3,767 words) - 15:43, 22 July 2014
- ...Further details on the definition of these parameters are available in {{PlanckPapers|planck2013-p03d}}.18 KB (805 words) - 14:32, 23 July 2014
- ...from each of Planck's nine frequency channels. It is fully described in {{PlanckPapers|planck2013-p05}}. ...are based on aperture photometry, PSF fitting and Gaussian fitting (see {{PlanckPapers|planck2013-p05}} for a detailed description of these additional photometrie12 KB (1,879 words) - 16:37, 23 July 2014
- {{PlanckPapers|rosset2010}}. The thermometers are ...e the Q and U Stokes parameters with minimal correction for the pointing {{PlanckPapers|rosset2010}}. Residual systematics will come from the differences between t13 KB (2,126 words) - 15:54, 22 July 2014
- ...is given in the appropriate LFI {{PlanckPapers|planck2013-p02d}} and HFI {{PlanckPapers|planck2013-p03c}} papers. Relevant details of the processing steps are give23 KB (3,381 words) - 12:28, 28 August 2014
- ...arameter tables. Definitions, conventions and reference are contained in {{PlanckPapers|planck2013-p11}}. ...n into account when comparing with BBN results reported in Sect. 6.4. of {{PlanckPapers|planck2013-p11}}, which use an updated version for the neutron lifetime (an10 KB (1,566 words) - 17:32, 23 July 2014
- ...contains the information from the summary section of the HFI DPC paper {{PlanckPapers|planck2013-p03}} which describes the most important characteristics of the449 bytes (64 words) - 15:03, 23 July 2014
- ...ng strategy'', makes use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of [[File:AHF_353_OD389.png|thumb|400px|The 353 GHz detectors {{PlanckPapers|lamarre2010}} integration time after 389 Operational Days (the unit is seco16 KB (2,501 words) - 14:28, 22 July 2014
- ...e 1 below. All the details can be found in the LFI data processing paper {{PlanckPapers|planck2013-p02}}. ...ective beam. Those are the values used in the source extraction pipeline {{PlanckPapers|planck2013-p05}}.2 KB (296 words) - 16:20, 23 July 2014
- ...report a brief summary of these effects, all the details can be found in{{PlanckPapers|planck2013-p02a}}. ...aps. The CMB curve corresponds to the Planck best-fit model presented in {{PlanckPapers|planck2013-p08}}.'''16 KB (2,578 words) - 16:05, 23 July 2014
- ...sked Galactic plane and point sources using masks described in Sec. 3 of {{PlanckPapers|planck2013-p06}}. In particular, we have used the 70% Galactic mask for 44 ...ment between the observed spectra and the Planck Likelihood Code bestfit {{PlanckPapers|planck2013-p08}} when adding a simple foreground component to account for u2 KB (270 words) - 16:19, 23 July 2014
- ...nels. Details about the definition of colour corrections are provided in {{PlanckPapers|planck2011-1-6}}. As detailed in {{PlanckPapers|planck2011-1-4}}, one effect detected during the first survey was the daily59 KB (9,067 words) - 10:10, 23 July 2014
- ...h-<math>\ell</math> likelihoods are described, discussed and compared in {{PlanckPapers|planck2013-p08}}. ...Y}(\ell)</math> of the relative error on <math>B^{XY}_{\ell}</math> (see {{PlanckPapers|planck2013-p03c|1|HFI time response and beams paper}}), defined for <math>p25 KB (3,721 words) - 17:10, 23 July 2014
- See the Component Separation paper {{PlanckPapers|planck2013-p06}} for details.12 KB (1,894 words) - 16:38, 23 July 2014
- ...ntre frequency. A detailed description of the LFI instrument is given in {{PlanckPapers|bersanelli2010}}, and references therein.3 KB (479 words) - 16:15, 22 July 2014
- ...t (i.e. 2.2.1.2, 4.4.5, and 4.6), as well as the Spectral Response Paper {{PlanckPapers|planck2013-p03d}} for details of the derivation of the detector spectra and ...dpass routine. Details of the unit conversion equations are available in {{PlanckPapers|planck2013-p03d}}.28 KB (4,680 words) - 10:21, 2 October 2014
- In {{PlanckPapers|planck2013-p03c}} we consider two models of the beam in order to better und ...cessing (see [[Frequency_Maps#HFI_processing | here]] or Section 3.11 of {{PlanckPapers|planck2013-p03}} for more info). We use JPL Horizons ephemerides to determi33 KB (5,387 words) - 14:27, 23 July 2014
- All the details can be found in {{PlanckPapers|planck2013-p06}}. ...isotropy map. These are the maps used in the component separation paper {{PlanckPapers|planck2013-p06}}.55 KB (8,302 words) - 09:26, 20 June 2016
- ...detector transfer function, which is complex in the Fourier domain (see {{PlanckPapers|planck2013-p03c}}). This phase shift was not measured during normal operati ...e radiometer electronics box assembly (REBA) as discussed more fully in {{PlanckPapers|planck2013-p03}}.17 KB (2,628 words) - 16:32, 23 July 2014
- For more information, see {{PlanckPapers|planck2011-1-1}}. For more information, see {{PlanckPapers|tauber2010a}}.14 KB (2,142 words) - 14:23, 22 July 2014