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- ;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 pair10 KB (1,542 words) - 09:41, 2 February 2018
- :[[HFI design, qualification, and performance]] :[[HFI cryogenics]]2 KB (165 words) - 17:42, 29 January 2015
- ...are averaged and transmitted to the ground. The TOI data delivered in the HFI products are made up of these averaged values, with the raw signal of a bol ..., since the users should not expect to be able to improve this part of the processing.1 KB (169 words) - 14:55, 23 May 2015
- ...interesting for characterization purposes (see also the [[HFI-Validation | data validation]] section), though some are also useful for the study of source For this (2018) release, HFI is providing a more limited subset of maps that include the full channel ma133 KB (19,918 words) - 11:57, 14 December 2022
- ...it is obtained, followed by a description of the FITS file containing the data and associated information. ...we do not release parametric temperature foreground products from the 2018 data set, but rather recommend continued usage of the 2015 temperature model. Fo107 KB (15,543 words) - 17:33, 22 October 2021
- This page is intented to provide complementary figures to those of the 2017 HFI DPC paper ({{PlanckPapers|planck2016-l03}}). ...unction of ring numbers. Blue line shows the solved gain variation for the data and grey ones show 10 realizations drawn within the uncertainties of the AD7 KB (1,208 words) - 11:31, 28 November 2017
- ...arts is intended to allow users to use the existing products to create new data. ...g the user with several tools to create a map cutout from the time-ordered data.61 KB (9,846 words) - 08:09, 27 August 2019
- * [[Planets related data | Planet-related data]] To support the interpretation of these data, these products are accompanied by:3 KB (425 words) - 12:19, 12 July 2018
- {{DISPLAYTITLE:HFI systematic effects}} ...es that needed to be tracked to verify that they were not compromising the data. While these are discussed in appropriate sections, here we gather the syst10 KB (1,498 words) - 07:38, 18 January 2019
- ...mplates; and the second iteration applies these and other corrections. HFI processing includes cosmic-ray glitch removal and bolometric transfer-function deconvo [[File:Preproc_hfi.png|800px|frameless|left|HFI preprocessing subpipeline]]1 KB (151 words) - 11:15, 22 June 2021
- ...PLA as agreed between ESA and the BeyondPlanck project reprocessing Planck data. Please note that these products have not been produced by the Planck Colla .../wiki.cosmos.esa.int/planck-legacy-archive/index.php/Main_Page Planck LFI] data within a self-consistent end-to-end Bayesian framework, in which both instr25 KB (3,590 words) - 09:35, 15 February 2023
- ...n the PLA as agreed between ESA and the Sroll2 project reprocessing Planck data. Please note that these products have not been produced by the Planck Colla ...ssociated errors have also been corrected based on the redundancies in the data and their residual levels characterized with simulations.10 KB (1,475 words) - 11:48, 13 June 2023