.. include:: ../../clsubstitutions.txt .. _selclProbDet: Probability of Cluster Detection Output Product ================================================== $SetSchemaPath le3/cl/euc-le3-cl-sel-probdet.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:** * SelectionFunction **Consumers** * Random .. PECreatorEnd Processing Function using the products _______________________________________ .. PFUsingStart * PF-LE3-CL * SWG-CL .. PFUsingEnd Proposed for inclusion in EAS/SAS _________________________________ .. IncludeInSASStart This product is proposed for inclusion in the SAS: Yes This product will be used by SWG and by downstream CL PFs. .. IncludeInSASEnd Data Product Elements _________________________ .. DataProductElementsStart $PrintDataProductElements .. DataProductElementsEnd Detailed Description of the Data Product ____________________________________________ .. DetailedDescStart This HDU gives the probability that a cluster with a richness lambda_true and a redshift_true is detected with at lambda_obs and redshift_obs, , and the associated statistical errors. These two datasets appear in two distinct HDUs, with identical header content and identical table format. Keywords ++++++++ These keywords should define the sky area, the quantities associated with the clusters detection, and the associated selection cuts from which the subsample is built. The default scheme is that the TRUE and OBS quantities have the same binning (TBC). - **AREA_MASK**: Reference to a visibility or footprint mask defining the target sky area - **Z_KEY**: Name of the redshift column used for the subsample - **RICHNESS_KEY**: Name of the richness column (i.e. LAMBDA) used for the subsample - **Z_TRUE_START**: Lower value of binning in Z_TRUE - **Z_TRUE_END**: Upper value of binning in Z_TRUE - **Z_TRUE_STEP**: Step value of binning in Z_TRUE - **Z_OBS_START**: Lower value of binning in Z_OBS - **Z_OBS_END**: Upper value of binning in Z_OBS - **Z_OBS_STEP**: Step value of binning in Z_OBS - **LAMBDA_TRUE_START**: Lower value of binning in LAMBDA_TRUE - **LAMBDA_TRUE_END**: Upper value of binning in LAMBDA_TRUE - **LAMBDA_TRUE_STEP**: Step value of binning in LAMBDA_TRUE - **LAMBDA_OBS_START**: Lower value of binning in LAMBDA_OBS - **LAMBDA_OBS_END**: Upper value of binning in LAMBDA_OBS - **LAMBDA_OBS_STEP**: Step value of binning in LAMBDA_OBS Tables ++++++ Each of these two tables has NBins(LAMBDA_TRUE) columns and NBins(Z_TRUE) lines. Each table cell contains a matrix oof NBins(LAMBDA_OBS columns and NBins(Z_OBS) lines. *First HDU:* - **PROB_LAMBDA_Z_OBS_TRUE** : Probability to detect a hypothetical cluster of richness LAMBDA_OBS and redshift Z_OBS, as a function of quantities LAMBDA_TRUE and Z_TRUE Equivalent table from XML: $PrintHDUTableContents fit/euc-le3-cl.xml le3.cl.sel.output.probdet PROB_LAMBDA_Z_OBS_TRUE *Second HDU:* - **ERR_PROB_LAMBDA_Z_OBS_TRUE** : Statistical error on the detection probability **PROB_LAMBDA_Z_OBS_TRUE** Equivalent table from XML: $PrintHDUTableContents fit/euc-le3-cl.xml le3.cl.sel.output.probdet ERR_PROB_LAMBDA_Z_OBS_TRUE .. DetailedDescEnd