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Information and status page for Herschel footprint re-generationThis page compiles the information for the footprint generation using the astrometry information from the latest bulk-reprocessed data (HIPE 14.x).Ancillary Files | ||||||||
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< < | The header and pointing parameter files extracted for each obsid have been stored at the following temporary area in the Herschel legacy repository: http://archives.esac.esa.int/hsa/legacy/other/.footprint/ ![]() Headers and pointing material are in two different sub-directories. Note that the PACS-P pointing stuff is really big (100 Gb). In the PACS-P pointing archive there are also about 1000 obsids for which the generation of pointing information failed - I am assuming that this is because they are FAILED observations that did not generate the necessary products where to extract the needed information. Also added is a text file with some "release" notes, explaining the inputs files that were used. The following remarks apply to the generation of the above files: PARALLEL mode: | |||||||
> > | The header and pointing parameter files extracted for each obsid have been stored at the following temporary area in the Herschel legacy repository: http://archives.esac.esa.int/hsa/legacy/other/.footprint/ ![]() Headers and pointing material are in two different sub-directories ( headerFiles ![]() ![]() Also added is a text file with some "release" notes, explaining the inputs files that were used. The following remarks apply to the generation of the above files: PARALLEL mode: | |||||||
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> > | Information and status page for Herschel footprint re-generationThis page compiles the information for the footprint generation using the astrometry information from the latest bulk-reprocessed data (HIPE 14.x).Ancillary FilesThe header and pointing parameter files extracted for each obsid have been stored at the following temporary area in the Herschel legacy repository:http://archives.esac.esa.int/hsa/legacy/other/.footprint/ ![]() Headers and pointing material are in two different sub-directories. Note that the PACS-P pointing stuff is really big (100 Gb). In the PACS-P pointing archive there are also about 1000 obsids for which the generation of pointing information failed - I am assuming that this is because they are FAILED observations that did not generate the necessary products where to extract the needed information. Also added is a text file with some "release" notes, explaining the inputs files that were used. The following remarks apply to the generation of the above files: PARALLEL mode:
Malformed footprints from previous releaseIn the previous release of the footprint, we identified 666 malformed footprints:
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