.. include:: ../../idsubstitutions.txt .. _VMPZIDMOCDepth: Output Product: MOC Depth Map =============================== $SetSchemaPath le3/id/vmpz/out/euc-le3-id-vmpz-MOCDepthMap.xsd Data Product Name __________________ .. DataProductNameStart $PrintDataProductName .. DataProductNameEnd Data Product Custodian _______________________ .. DataProductCustodianStart $PrintDataProductCustodian .. DataProductCustodianEnd Name of the Schema File ________________________ .. NameSchemaStart $PrintSchemaFilename .. NameSchemaEnd Last Edited for DPDD Version ____________________________ .. DpddVersionlTagStart 1.1 .. DpddVersionTagEnd Processing Elements Creating / Updating / Using the Product ___________________________________________________________ .. PECreatorStart **Creators:** * VMPZ_Main (LE3_VMPZ_ID_Main) **Consumers:** * VMPZ_Visibility (LE3_VMPZ_ID_Visibility) .. PECreatorEnd Processing function using the data product _____________________________________________ .. PFUsingStart * 2PCF-WL, PK-WL, 2PCF-GC, 3PCF-GC, PK-GC, DET-CL, PROF-CL, VMSP-ID * SWG-GC, SWG-WL, SWG-CL .. PFUsingEnd Proposed for inclusion in EAS/SAS _________________________________ .. IncludeInSASStart This product is proposed for inclusion in SAS: yes This product is used by different PFs in OU-LE3 and expected to be used in scientific analysis in SWG-GC, SWG-WL and SWG-CL. .. IncludeInSASEnd Data Product Elements ______________________ .. DataProductElementsStart $PrintDataProductElements .. DataProductElementsEnd Detailed Description of the Data Product _________________________________________ .. DetailedDescStart This output product is a partial MOC map collecting the depth maps. It includes the **DepthMapMOC** metadata, a container with a FITS file (of type le3.id.vmpz.mocdepthmap) describing the depth map for the survey in MOC 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, `spatialFootprint `_). Finally, the mask parameters **DepthMapMOCParams** 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: $PrintPrimaryHeader fit/euc-le3-id.xml le3.id.vmpz.mocdepthmap #. **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] #. **BITSEL**: identifier of the bit of combination of bits used in the depth map (e.g. 0 for least significant bit,..,18) [StringKeyword] #. **DEPTHEST**: estimator used for depth computation [StringKeyword] and basic software parameters: #. **SOFTNAME**: name of software used [StringKeyword] #. **SOFTVERS**: version of software used [StringKeyword] Partial MOC Footprint Table (First Extension, Binary Table) +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ The following keywords are used to describe what MOC conventions are followed: $PrintHDUTableContents fit/euc-le3-id.xml le3.id.vmpz.mocdepthmap DEPTH_MAP #. **TTYPE1** (= 'UNIQ') [StringKeyword] #. **TFORM1** (= 'K') [StringKeyword] #. **TTYPE2** (= 'WEIGHT') [StringKeyword] #. **TFORM2** (= 'E') [StringKeyword] #. **PIXTYPE** (= 'HEALPIX') [StringKeyword] #. **ORDERING** (= 'NUNIQ') [StringKeyword] #. **COORDSYS** (= 'C'=celestial, 'E'=ecliptic or 'G'=galactic) [StringKeyword] #. **MOCORDER** (best HEALPix order) [IntegerKeyword] #. **MOCTYPE** [StringKeyword] #. **DATE** [StringKeyword] #. **EXTNAME** (= 'DEPTH_MAP') [StringKeyword] The table is then expected to contain the following columns: #. **UNIQ**: index of pixel [K, int64] #. **WEIGHT**: (floating-point) weight associated to pixel indicating the depth [E, float32] .. note:: Should add keywords for galaxy type if input parameters .. DetailedDescEnd