Difference between revisions of "DatesObs"
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| − | + | == Overview == | |
| + | |||
The DatesObs files are not official Planck products but have been made available for the convenience of the community. They contain timing information split by survey, gridded by HEALPIX pixel, and sampled by UTC day. They are intended for investigation of inter-survey source variability, comparison with external observations, and understanding of the survey strategy. | The DatesObs files are not official Planck products but have been made available for the convenience of the community. They contain timing information split by survey, gridded by HEALPIX pixel, and sampled by UTC day. They are intended for investigation of inter-survey source variability, comparison with external observations, and understanding of the survey strategy. | ||
| − | + | == File Format == | |
| − | There are | + | |
| − | + | There are 54 files; 6 HFI bands x 5 surveys & 3 LFI bands x 8 surveys. They are named: | |
| + | |||
| + | ''HFI_DatesObs_fff_Nside_R2.nn_survey_k.fits.gz'' | ||
| + | |||
| + | where ''fff'' is the usual 3-digit description of the channel frequency. | ||
| + | |||
| + | The files themselves are in FITS format, and gzipped, with data in the first extension | ||
* RING-ordered HEALPIX | * RING-ordered HEALPIX | ||
* NSIDE 1024 for LFI, and 2048 for HFI | * NSIDE 1024 for LFI, and 2048 for HFI | ||
| Line 15: | Line 22: | ||
Unobserved pixels have been left blank. | Unobserved pixels have been left blank. | ||
| − | + | == Generation == | |
The DATESOBS files were generated by projecting the line-of-sight of each detector onto the sky on a ring-by-ring basis. Inputs were the satellite spin-axis and the opening angle of each detector. Position is thus accurate to nearest pixel center and timing to the start of each ring - rings over midnight are only counted for the day in which they begin. | The DATESOBS files were generated by projecting the line-of-sight of each detector onto the sky on a ring-by-ring basis. Inputs were the satellite spin-axis and the opening angle of each detector. Position is thus accurate to nearest pixel center and timing to the start of each ring - rings over midnight are only counted for the day in which they begin. | ||
| Line 25: | Line 32: | ||
Detectors not used in production of the frequency maps were excluded. | Detectors not used in production of the frequency maps were excluded. | ||
| − | Finally the data have been masked by the per-survey SkyMap hit-maps in order to remove areas which were flagged during the processing (mainly planet crossings). | + | Finally the data have been masked by the per-survey SkyMap hit-maps in order to remove areas which were flagged during the processing (mainly planet crossings). No ring cuts were applied so some anomalous rings are included. |
| + | |||
| + | == HEALPix IDL read_fits_map == | ||
| + | |||
| + | Note the datesobs files cannot be read by HEALPix's IDL read_fits_map routine as it is not expecting string content. There is no problem with the standard AstroLib mrdfits. | ||
| + | |||
| + | [[file:numobs.png|thumb|600px|center|Full-sky map of the number of observations in the first survey.]] | ||
| − | [[ | + | [[Category:Mission products|013]] |
Latest revision as of 02:30, 22 February 2017
Overview[edit]
The DatesObs files are not official Planck products but have been made available for the convenience of the community. They contain timing information split by survey, gridded by HEALPIX pixel, and sampled by UTC day. They are intended for investigation of inter-survey source variability, comparison with external observations, and understanding of the survey strategy.
File Format[edit]
There are 54 files; 6 HFI bands x 5 surveys & 3 LFI bands x 8 surveys. They are named:
HFI_DatesObs_fff_Nside_R2.nn_survey_k.fits.gz
where fff is the usual 3-digit description of the channel frequency.
The files themselves are in FITS format, and gzipped, with data in the first extension
- RING-ordered HEALPIX
- NSIDE 1024 for LFI, and 2048 for HFI
They contain two fields:
- DATESOBS - string - comma-separated list of UTC days in YYMMDD format on which the pixel was observed
- NUMOBS - integer - the number of UTC days on which the pixel was observed
Unobserved pixels have been left blank.
Generation[edit]
The DATESOBS files were generated by projecting the line-of-sight of each detector onto the sky on a ring-by-ring basis. Inputs were the satellite spin-axis and the opening angle of each detector. Position is thus accurate to nearest pixel center and timing to the start of each ring - rings over midnight are only counted for the day in which they begin.
Note no beam information was used, just closest line-of-sight. The list of dates within a beam width is thus the union of the date information for all pixels within the appropriate area.
Pixels were counted observed if hit by a single detector within each instrument band; there was no consideration of intra-band coverage.
Detectors not used in production of the frequency maps were excluded.
Finally the data have been masked by the per-survey SkyMap hit-maps in order to remove areas which were flagged during the processing (mainly planet crossings). No ring cuts were applied so some anomalous rings are included.
HEALPix IDL read_fits_map[edit]
Note the datesobs files cannot be read by HEALPix's IDL read_fits_map routine as it is not expecting string content. There is no problem with the standard AstroLib mrdfits.
Universal Time Coordinate(d)
(Planck) High Frequency Instrument
(Planck) Low Frequency Instrument
Flexible Image Transfer Specification
(Hierarchical Equal Area isoLatitude Pixelation of a sphere, <ref name="Template:Gorski2005">HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere, K. M. Górski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke, M. Bartelmann, ApJ, 622, 759-771, (2005).
