Search results
Create the page "LFI data processing: Introduction" on this wiki! See also the search results found.
- ...descriptions of all the Planck products, including the 2013, 2015 and 2018 data releases. Previous instances of the Explanatory Supplement (2013 and 2015), #[[Introduction|Introduction]]5 KB (588 words) - 09:21, 6 August 2018
- ...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). == Introduction ==28 KB (4,118 words) - 16:15, 15 October 2015
- == Introduction == ...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 packa5 KB (484 words) - 10:47, 18 October 2012
- == Introduction == data of a quality adequate to measure the CMB signal and distinguish it from oth16 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 from4 KB (601 words) - 14:24, 22 July 2014
- ...angle from the spin axis. 545 GHz, 857 GHz, 143 GHz bolometers as well as LFI 25-26 radiometers have a slightly smaller bore-sight angle, while the other == Data gap recoveries ==16 KB (2,501 words) - 14:28, 22 July 2014
- ...is delivered as a tarfile and contains a detailed instruction manual. The data and software file requirements are provided below along with basic use inst ...ro</tt>: a routine to get the desired detector level spectral transmission data (HFI) and output in a structure format used by the other routines.28 KB (4,680 words) - 10:21, 2 October 2014
- == Introduction and Summary == ...idual detectors are known exactly a priori, we must calibrate using flight data.17 KB (2,628 words) - 16:32, 23 July 2014
- ...ssing radiation from the sky onto a focal plane shared by detectors of the LFI and HFI, operating at 20K and 0.1K respectively; a telescope baffle that si |Planck operated for 32 months with both instruments; the LFI continues surveying the sky14 KB (2,142 words) - 14:23, 22 July 2014