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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
  • == HFI spectral response pre-flight spectral characterization data processing and Fourier transformation == ...and can thus be averaged together. An example of a combined interferogram data set is illustrated in the figure below where the central portions of the re
    8 KB (718 words) - 16:03, 22 July 2014

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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), ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]]
    5 KB (588 words) - 09:21, 6 August 2018
  • ...frequency amplification stage, detector diodes and all the electronics for data acquisition and bias supply. ...less hydrogen sorption cooler, which also provides 18 K pre-cooling to the HFI helium J-T cooler. Two sorption cooler units are included in the flight har
    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]]'' ; [[TOI_processing LFI| TOI processing]]: ''[[TOI_processing LFI#Overview|Overview]] • [[TOI_processing LFI#ADC
    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
  • This section describes products that require special processing. Only one such product is available at this time; this section will be expa Also, the table below gives the lensing curl-mode power spectrum data used to produce Figure A2 of {{PlanckPapers|planck2013-p12}}:
    7 KB (921 words) - 17:34, 23 July 2014
  • ...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''' [HFI meaning]: For a single detector, the absolute calibration is gain factor be * '''detector set''' [HFI meaning]: a detector set (aka detset aka quad) is a combinaison of two pair
    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 HFI Consortium, Principal Investigator J.L. Puget of the Institut d'Astrophysiq
    9 KB (1,372 words) - 08:30, 21 September 2012
  • In terms of data processing, the HFI ground segment handles two types of data, both made available via the MOC: * telemetry data transmitted from the satellite. These come from the different subsystems of
    13 KB (1,976 words) - 13:53, 23 July 2014
  • ...and a variance map. All maps are in Healpix format, with Nside of 2048 for HFI and of 1024 for LFI, in Galactic coordinates, and Nested ordering. The thr ...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
  • ...rview of the map-making and photometric calibration procedures used by the HFI DPC to build detector and frequency maps. This processing and its performances are described in {{PlanckPapers|planck2013-p03}} and {
    11 KB (1,710 words) - 14:31, 23 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 dis ...would be named ''LFI_2_3_someName.png'' and a jpeg figure uploaded by the HFI to be displayed in section 6.4.3.1 would be named ''HFI_2_3_someOtherName.j
    31 KB (5,455 words) - 18:41, 16 March 2013
  • = HFI Detector Spectral Response = ...dband Fourier transform spectrometer (FTS) measurements conducted with the HFI focal plane assembly as described above, and includes a waveguide model for
    58 KB (7,853 words) - 15:51, 5 October 2012
  • ...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
  • ...eters, so as to keep the noise properties as uncorrelated as possible. The processing involves modifying the TOI itself for what concerns the conversion to absor ...ion frequency of facq=180.373700+-0.000050 Hz. There are almost no missing data in the TOIs, except for few hundred samples of 545 and 857 GHz TOIs which w
    18 KB (2,712 words) - 13:55, 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

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