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- AMo: this page is to be renamed "Frequency maps", and idem for its category75 bytes (14 words) - 11:40, 14 August 2012
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- ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] ###[[HFI_cold_optics_%26_spectral_response | HFI cold optics and spectral response]]8 KB (994 words) - 08:41, 4 December 2023
- ...ter all, it is not entirely unexpected that a user interested in frequency maps may also be interested in other types of map. Here DPC is one of HFI or LFI, x_x_x_x the section number for the page where the image will be dis36 KB (6,203 words) - 01:01, 25 September 2014
- ...to the warm (roughly 300 K) back-end unit (BEU) containing a further radio frequency amplification stage, detector diodes, and all the electronics for data acqu ...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 har50 KB (7,843 words) - 15:28, 4 July 2018
- ;HFI design, qualification and performance :[[HFI design, qualification, and performance]]2 KB (261 words) - 15:54, 26 March 2014
- ...ations (circle), the end of the nominal mission (triangle), and the end of HFI data acquisition (diamond). The orbital periodicity is 6 months. The distan ...scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.37 KB (5,882 words) - 09:23, 10 July 2018
- ...ps at specific frequencies into more scientific products, like catalogues, maps, and spectra of astrophysical components. L3 can rely on simulation provide ...ze:150%">'''Level 2: converting temporal information into clean calibrated maps'''</span>4 KB (627 words) - 01:28, 23 May 2015
- ...on|Photometric calibration]] • [[Map-making#Building_of_Maps|Building of Maps]] • [[Map-making#Noise_properties|Noise properties]] • [[Map-making#Zo ...[[HFI-Validation#Simulations_versus_data|Simulations versus data]] • [[HFI-Validation#Systematics_Impact_Estimates|Systematics Impact Estimates]]''8 KB (1,104 words) - 15:32, 4 July 2018
- ...r the first time the realistic simulation of instrumental effects for both HFI and LFI. Moreover these simulated systematic effects are processed in the t ...0 realizations of lensed scalar CMB convolved with effective beams per HFI frequency,114 KB (17,146 words) - 09:49, 21 February 2022
- ...color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are |rowspan="6" align="center" | HFI83 KB (8,209 words) - 12:21, 5 February 2015
- ...ck2016-l02=[http://arxiv.org/abs/1807.06206'''Planck 2018 results. II. Low Frequency Instrument data processing'''], Planck Collaboration, 2020, A&A, 641, A ...2018 results. III. High Frequency Instrument data processing and frequency maps'''], Planck Collaboration, 2020, A&A, 641, A3.67 KB (9,112 words) - 13:20, 25 September 2020
- ...single-frequency source catalogues extracted from the Planck full-mission maps in intensity and polarization (LFI_SkyMap_0??_1024_R2.01_full.fits and HFI_ ...ur observations for HFI channels. The relevant properties of the frequency maps and main parameters used to generate the catalogues are summarized in Table142 KB (20,039 words) - 12:58, 26 January 2021
- ...ng a cross quasi maximum likelihood algorithm (QML) on the 100 and 143 GHz maps and validated against high fidelity end-to-end simulations. ...o release the <i>BB</i>, and <i>EB</i> power spectra derived from the same maps. Error bars are given as the 68% confidence intervals as derived from the F118 KB (17,535 words) - 10:05, 11 May 2021
- ...k Collaboration: ''Planck intermediate results. LVII. Joint Planck LFI and HFI data processing'', [https://www.aanda.org/articles/aa/abs/2020/11/aa38073-2 ...ization can be captured with templates derived from the other (foreground) frequency channels. The calibration for the CMB frequencies is thus based on temperat8 KB (1,239 words) - 11:51, 22 June 2021
- ...ption of the product, including e.g. figures related to the contents (e.g. maps, tables), and some explanation of its scientific meaning. If there are scie Auto and cross angular power spectra for the 13 detset maps available at 100, 143 and 217GHz are provided in the Planck Legacy Archive3 KB (478 words) - 18:38, 26 February 2013
- {{DISPLAYTITLE:2018 CMB maps}} ...These products are derived from some or all of the nine frequency channel maps using different techniques and, in some cases, using other constraints from124 KB (18,807 words) - 18:58, 20 March 2023
- == 2018 Lensing maps == : Baseline lensing potential estimates from SMICA DX12 CMB maps. Provided are temperature-only (TT), polarization-only (PP) and minimum-var37 KB (5,494 words) - 12:25, 10 July 2019
- **''HFI'' - For a single detector, the absolute calibration is the gain factor betw * '''detector set''': for HFI, a detector set (also known as "detset" or "quad") is a combinaison of two7 KB (1,093 words) - 06:30, 24 May 2015
- ...t combining the two timelines section into one, and idem for the frequency maps. I have discussed this with A.Zacchei who agrees.255 bytes (44 words) - 12:04, 3 August 2012
- ...PlanckPapers|planck2014-a03}} and {{PlanckPapers|planck2016-l02}}, and for HFI, to {{PlanckPapers|planck2014-a08}}. ...timelines are applicable to all data releases. The Calibrated timelines of HFI are applicable to both 2015 and 2017 releases; note that for the 2017 relea40 KB (6,006 words) - 11:30, 22 June 2021
- ! There are no single detector maps in the first release. ...of 1024 for LFI, in Galactic coordinates, and Nested ordering. The three maps will be packaged into a FITS files with a single ''BINTABLE'' extension con5 KB (484 words) - 10:47, 18 October 2012
