.. _VMPZIDHEALPixFootprintMask: .. include:: ../../idsubstitutions.txt Output Product: HEALPix Footprint Mask -------------------------------------- Data product name ================= .. DataProductNameStart VMPZIDHEALPixFootprintMask .. DataProductNameEnd Data product custodian ====================== .. DataProductCustodianStart VMPZ-ID .. DataProductCustodianEnd Data model tag ============== .. DataModelTagStart |ML2A2BF| .. DataModelTagEnd Name of the Schema file ======================= .. NameSchemaStart |ML2A2BF| .. NameSchemaEnd Schema documentation tag ======================== .. SchemaDocTagStart |ML2A2BF| .. SchemaDocTagEnd Data product elements ===================== .. DataProductElementsStart |ML2A2BF| .. DataProductElementsEnd Processing Element(s) creating/using the data product ===================================================== .. PECreatorStart VMPZ-ID, (CM-)PK-WL .. PECreatorEnd Processing function using the data product ========================================== .. PFUsingStart LE3 .. PFUsingEnd Detailed description of the data product ======================================== .. DetailedDescStart This output product is essentially the footprint of the survey for a given band/instrument. The **FootprintMaskHealpix** metadata includes a container with a FITS file (of type le3.id.vmpz.healpixfootprintmask) describing the footprint for the survey in partial HEALPix format, for a given observed band/instrument (Euclid/EXT), and a raw description with polygons of the envelope of the sky covered is added as well to ease future queries on the product (**SpatialCoverage** metadata, see `spatialFootprint `_). Finally, the mask parameters **FootprintMaskHealpixParams** can optionally be associated to the product. Keywords (Primary HDU) ++++++++++++++++++++++ The primary HDU is expected to contain the following keywords, characterizing important parameters of the input product: #. **DATE-OBS**: start of observation with format 'yyyy-mm-ddThh:mm:ss.sss' [StringKeyword] #. **DATE-END**: end of observation with format 'yyyy-mm-ddThh:mm:ss.sss' [StringKeyword] #. **TELESCOP**: name of the telescope [StringKeyword] #. **INSTRUME**: name of the instrument [StringKeyword] #. **FILTER**: name of the filter [StringKeyword] #. **FILTLST**: selection of filter if intersection of multiple footprints [StringKeyword] #. **TILEID**: identifier of the MER Tile processed (-1 if multiple Tiles) [IntegerKeyword] #. **LISTID**: identifier of a MER list of tiles product (-1 if single Tile) [StringKeyword] #. **NSIDE_WK**: Nside parameter used for frame->HEALPix [StringKeyword] and basic software parameters: #. **SOFTNAME**: name of software used [StringKeyword] #. **SOFTVERS**: version of software used [StringKeyword] Partial HEALPix Footprint Table (First Extension, Binary Table) +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ The following keywords are used to describe what HEALPix conventions are followed: #. **TTYPE1** (= 'PIXEL') [StringKeyword] #. **TFORM1** (= 'K') [StringKeyword] #. **TTYPE2** (= 'WEIGHT') [StringKeyword] #. **TFORM2** (= 'E') [StringKeyword] #. **PIXTYPE** (= 'HEALPIX') [StringKeyword] #. **ORDERING** (= 'RING' or 'NESTED') [StringKeyword] #. **COORDSYS** (= 'C'=celestial, 'E'=ecliptic or 'G'=galactic) [StringKeyword] #. **EXTNAME** (= 'FOOTPRINT_MASK') [StringKeyword] #. **NSIDE** [IntegerKeyword] #. **INDEXSCHM** (= 'EXPLICIT') [StringKeyword] #. **OBJECT** (= 'PARTIAL') [StringKeyword] The table is then expected to contain the following columns: #. **PIXEL**: index of pixel [K, int64] #. **WEIGHT**: weight associated to pixel in [0,1] indicating the fraction of the pixel actually covered by the footprint (1: fully not observed regions) [E, float32] .. DetailedDescEnd