.. include:: ../../wlsubstitutions.rst .. _twoDMassConvergenceSingleCluster: Output Product: E/B Convergence Maps for a single Cluster --------------------------------------------------------- Data product name ================= .. DataProductNameStart twoDMassConvergenceSingleCluster .. DataProductNameEnd Data product custodian ====================== .. DataProductCustodianStart 2D-MASS-WL .. DataProductCustodianEnd Data model tag ============== .. DataModelTagStart |2BF| .. DataModelTagEnd Name of the Schema file ======================= .. NameSchemaStart euc-test-le3-wl-twodmass-ConvergenceSingleCluster.xsd .. NameSchemaEnd Schema documentation tag ======================== .. SchemaDocTagStart :emphasis:`Data product documentation:` Data Product for twoDMassConvergenceSingleCluster. :emphasis:`Documentation for data product element dpdTwoDMassConvergenceSingleCluster:` This product contains FITS images with convergence/SNR maps around a single massive cluster stored in a FITS file. :emphasis:`Documentation for data product element Header:` The generic header of the product :emphasis:`Documentation for data product element Data:` The data of the product .. SchemaDocTagEnd Data product elements ===================== .. DataProductElementsStart Header of type: sys:genericHeader Data of type: wl2dmass:twoDMassConvergenceSingleCluster QualityFlags of type: dqc:sqfPlaceHolder Parameters of type: ppr:genericKeyValueParameters .. DataProductElementsEnd Processing Element(s) creating/using the data product ===================================================== .. PECreatorStart 2D-MASS-WL .. PECreatorEnd Processing function using the data product ========================================== .. PFUsingStart SGS pipeline output product to be used by SWGs .. PFUsingEnd Detailed description of the data product ======================================== .. DetailedDescStart This output product contains in a FITS file data arrays with as HDUs the noisy/denoised E/B modes, SNR maps for a patch centered on a detected (and sufficiently massive) cluster with an associated spatial footprint (see `spatialFootprint here `_). A *ClusterID* XML field as well as an optional *ClusterMass* field are also added to the product. For the FITS product: Keywords (Primary HDU) ++++++++++++++++++++++ Important parameters of the product are stored, such as the world coordinate system (see A&A 395, 1077-1122 (2002)): #. **WCSAXES** = "2": number of axes in World Coordinate System [int] #. **CRPIX1**: pixel number of reference pixel in first dimension [double] #. **CRPIX2**: pixel number of reference pixel in second dimension [double] #. **PC1_1**: component (1,1) of the coordinate transformation matrix [double] #. **PC1_2**: component (1,2) of the coordinate transformation matrix [double] #. **PC2_1**: component (2,1) of the coordinate transformation matrix [double] #. **PC2_2**: component (2,2) of the coordinate transformation matrix [double] #. **CDELT1**: coordinate increment at reference point (1st dim) [double] #. **CDELT2**: coordinate increment at reference point (2nd dim) [double] #. **CUNIT1**: unit of first coordinate values (CRVAL, CDX_X) [string] #. **CUNIT2**: unit of second coordinate value (CRVAL, CDX_X) [string] #. **CTYPE1**: first parameter for reference (e.g. RA---TAN for right ascension in gnomonic projection) [string] #. **CTYPE2**: second parameter for reference (e.g. DEC--TAN for declination in gnomonic projection) [string] #. **CRVAL1**: first reference pixel value for CTYPE1 [double] #. **CRVAL2**: second reference pixel value for CTYPE2 [double] #. **LONPOLE**: native longitude of celestial pole [double] #. **LATPOLE**: native latitude of celestial pole [double] #. **RADESYS**: Coordinate system (e.g. 'FK5') [string] #. **EQUINOX**: equinox of celestial coordinate system (e.g. 2000) [string] #. **DATE-OBS**: start of observation with format 'yyyy-mm-ddThh:mm:ss.sss' [string] #. **DATE-END**: end of observation with format 'yyyy-mm-ddThh:mm:ss.sss' [string] and software parameters: #. **SHE_SOFT**: which SHE catalogue used [StringKeyword] #. **SOFTNAME**: software used to create the product [string] #. **SOFTVERS**: version of software [string] #. **PROJ**: projection used (gnomonic implemented) [string] #. **PWIDTH**: Patch Width [double] #. **PIXSIZE**: physical size of the pixels in the patch [double] #. **NITREDSH**: number of iteration to compute reduced shear [int] #. **STDREDSH**: standard deviation for Gaussian smoothing performed to compute the reduced shear (0 if no Gaussian smoothing) [double] #. **FDRREDSH**: false discovery rate threshold used to compute the reduced shear [double] #. **NITINP**: number of iteration for inpainting (0 if no inpainting) [int] #. **NSCINP**: number of scale for inpainting (0 if no inpainting) [int] #. **VARPERSC**: flag specifying if equal variance in/out masked area per scale [bool] #. **FBMODE**: flag specifying if B-Mode forced to 0 in the gaps [bool] #. **ADDBORD**: specify if border effect processing [bool] #. **DENTYPE**: denoising type (e.g. Gaussian, name of third party software) [string] #. **GAUSSSTD**: standard deviation for Gaussian smoothing (0 if no Gaussian smoothing) [double] #. **FDRVAL**: false discovery rate threshold [double] #. **NRESAMPL**: number of resampling for computing noise maps [int] #. **ZMIN**: minimum redshift considered [double] #. **ZMAX**: maximum redshift considered [double] #. **CL_ID**: ID of the cluster considered [string] #. **CL_MASS**: mass of the cluster [double] ArrayHDU (optional): Noisy convergence map ++++++++++++++++++++++++++++++++++++++++++ The following keywords are specified for each hdu: #. **EXTNAME** = "NOISY_KAPPA_PATCH" The image contains a 3 dimensional image containing the 2D noisy E/B modes. ArrayHDU (optional): Denoised convergence map +++++++++++++++++++++++++++++++++++++++++++++ The following keywords are specified for the second HDU: #. **EXTNAME** = "DENOISED_KAPPA_PATCH" The image contains a 3 dimensional image containing the 2D denoised E/B modes. ArrayHDU (optional): Galaxy Count map +++++++++++++++++++++++++++++++++++++ The following keywords are specified for each hdu: #. **EXTNAME** = "GALAXY_COUNT" The image contains an image with the number of galaxies per pixel in the maps (can serve to derive a noise level or to identify zones where inpainting has been performed- zone with no galaxy measured). ArrayHDU (optional): SNR map ++++++++++++++++++++++++++++ The following keywords are specified for each hdu: #. **EXTNAME** = "SNR_PATCH" The image contains a 3 dimensional image containing the 2D noisy E and B modes, the 2D denoised E and B modes if provided, and an image with the number of galaxies per pixel in the redshift bin (can serve to derive a noise level or to identify zones where inpainting has been performed - zones with no galaxy measured). .. DetailedDescEnd