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  • HFI/LFI common processing uses as basic input the maps at the nine frequencies covered by the two ins ...lihood code (of a particular theoretical <math>C(\ell)</math> given Planck data).
    464 bytes (69 words) - 21:13, 17 March 2013

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  • ...descriptions of all the Planck products, including the 2013, 2015 and 2018 data releases. Previous instances of the Explanatory Supplement (2013 and 2015), ##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span>
    5 KB (588 words) - 09:21, 6 August 2018
  • ...frequency amplification stage, detector diodes and all the electronics for data acquisition and bias supply. Best LFI noise performance is obtained with receivers based on InP High Electron Mob
    50 KB (7,790 words) - 10:04, 23 July 2014
  • ...ed by the LS, while L4 refers to delivering the DPC products to ESA. This processing relies on dedicated software and hardware infrastructures developed pre-lau ...d its co-papers provide the reference for the processing done for the 2013 data release.
    4 KB (619 words) - 13:50, 23 July 2014
  • ...etry handling]] • [[Pre-processing LFI#Auxiliary data handling|Auxiliary data handling]]'' ...Calibration]] • [[TOI_processing LFI#Noise|Noise]] • [[TOI_processing LFI#References|References]] ''
    7 KB (1,004 words) - 15:06, 23 July 2014
  • ...ta can be downloaded from the PLA Java interface (Windows -> Supplementary Data). The 2013 Planck data release is supported by a set of simulated maps of the model sky, by astrop
    28 KB (4,118 words) - 16:15, 15 October 2015
  • ...uency information. Future releases will take advantage of the full mission data and they will contain information on properties of sources not available in ...n {{PlanckPapers|planck2013-p02}} and {{PlanckPapers|planck2013-p03}}. The data consist of two complete sky surveys and 60% of the third survey. This impli
    30 KB (4,218 words) - 16:56, 23 July 2014
  • * '''calibration''': [LFI meaning]: absolute calibration refers to the 0th order calibration for each * '''DMC''' : Data Management Component, the databases used at the HFI and LFI DPCs
    7 KB (1,048 words) - 12:32, 28 August 2014
  • ...mission, and who participate in the scientific exploitation of the Planck data during the proprietary period, which nominally ends with the release of the *The LFI Consortium, Principal Investigator N. Mandolesi of the Istituto di Astrofis
    9 KB (1,372 words) - 08:30, 21 September 2012
  • ...ll maps are in Healpix format, with Nside of 2048 for HFI and of 1024 for LFI, in Galactic coordinates, and Nested ordering. The three maps will be packa ...lpix Nside of the map, the optional ''type'' indicates the subset of input data used, and ''mission'' indicates the coverage period, i.e., ''full'', ''nomi
    5 KB (484 words) - 10:47, 18 October 2012
  • ...nd of other products described elsewhere (see e.g., the [[HFI-Validation | data validation]] section). To help in further processing, there are also masks of the Galactic Plane and of point sources, each prov
    35 KB (5,220 words) - 13:00, 24 July 2014
  • Where DPC is one of HFI or LFI, x_x_x_x the section number for the page where the image will be displayed A png figure uploaded by the LFI to be displayed in section 2.3 would be named ''LFI_2_3_someName.png'' and
    31 KB (5,455 words) - 18:41, 16 March 2013
  • ...w the same overall structure, but will differ in the details. The type of data in the RIMO can be: ...keywords that mainly for internal use and no data. The different types of data are written into different BINTABLE (for parameters and tables) or IMAGE (f
    12 KB (1,821 words) - 16:42, 23 July 2014
  • data of a quality adequate to measure the CMB signal and distinguish it from oth about six 5 times for the HFI and 8 times for the LFI.
    16 KB (2,489 words) - 13:19, 22 July 2014
  • ...g (HK) data acquired by the satellite during the past 24 h. The downlinked data are typically 8 h; at MOC they are put onto a data server from
    4 KB (601 words) - 14:24, 22 July 2014
  • ...the [[The LFI DPC|LFI]] and also the [[HFI/LFI joint data processing|joint processing]]. [[Category:Data processing|000]]
    370 bytes (60 words) - 15:18, 3 July 2014
  • {{DISPLAYTITLE:TOI processing}} The LFI Level2 Pipeline analyzes each horn of the instrument separately, one pointi
    31 KB (4,941 words) - 15:14, 23 July 2014
  • {{DISPLAYTITLE:Pre-processing}} ...first processing level of the LFI DPC is the so called Level 1. The source data of the Level 1 software includes:
    14 KB (2,299 words) - 20:58, 17 March 2013
  • ...s described in the [[TOI processing#Thermal template for decorrelation|TOI processing]] section. ...or frequency. The removal of these interferences is addressed in the [[TOI processing#Thermal template for decorrelation|4K cooler lines variability]] section.
    5 KB (747 words) - 15:36, 22 July 2014
  • ...aking, or any other, validates the results of its work at each step of the processing, looking specifically for known issues. In addition, we do additional valid ...of "issues" which it needed to track and verify were not compromising the data. While these are discussed in appropriate sections, here we gather them tog
    25 KB (4,008 words) - 15:01, 23 July 2014
  • LFI maps were constructed with the Madam map-making code, version 3.7.4. The conversion was applied to the input pointing data, prior to the construction of the map.
    23 KB (3,368 words) - 15:56, 23 July 2014

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