.. include:: ../../clsubstitutions.txt .. _detclParameters: Detection Parameters Input Product for -------------------------------------------- Data product name ================= .. DataProductNameStart detclParameters .. DataProductNameEnd Data product custodian ====================== .. DataProductCustodianStart DET-CL .. DataProductCustodianEnd Data model tag ============== .. DataModelTagStart DpdLE3clCcpInputParams .. DataModelTagEnd Name of the Schema file ======================= .. NameSchemaStart test-le3-cl-ccp-params.xsd .. NameSchemaEnd Schema documentation tag ======================== .. SchemaDocTagStart This product contains the input parameters for DET-CL .. SchemaDocTagEnd Data product elements ===================== .. DataProductElementsStart :Header: type sys:genericHeader :Data: type cl:ccpParametersList :QualityFlags: type dqc:sqfPlaceHolder :Parameters: type ppr:genericKeyValueParameters .. DataProductElementsEnd Processing Element(s) creating/using the data product ===================================================== .. PECreatorStart DET-CL .. PECreatorEnd Processing function using the data product ========================================== .. PFUsingStart LE3, "DET-CL" pipeline .. PFUsingEnd Detailed description of the data product ======================================== .. DetailedDescStart This data product contains the list and description of the parameters used for the detection of the clusters. Keywords ++++++++ This XML file is expected to contain the following keywords in the data table HDU: KEYWORDS COMMON TO BOTH DETECTION CODES: GENERAL PARAMETERS: #. **MIN_Z**: lower limit of redshift range for cluster detection #. **MAX_Z**: upper limit of redshift range for cluster detection #. **MIN_RA**: Minimum RA of the area on which the run has to be performed [deg] #. **MAX_RA**: Maximum RA of the area on which the run has to be performed [deg] #. **MIN_DEC**: Minimum Dec of the area on which the run has to be performed [deg] #. **MAX_DEC**: Maximum Dec of the area on which the run has to be performed [deg] #. **SNR_THR**: the S/N threshold for extracting a detection KEYWORDS SPECIFIC TO AMICO DETECTION CODE: #. **CUBE_XY_STEP**: size of the RA and Dec bin [deg] #. **MAX_AREA_DEG**: Maximum area for a single tile on which AMICO can run [deg^2] #. **L_BORDER_DEG**: Size of the border defining the detection area [deg] KEYWORDS SPECIFIC TO PZWAV DETECTION CODE: #. **DZ**: half width of reach redshift slice #. **ZSTEP**: interval between slices #. **KRN_SCL1**: lower scale of kernel, in kpc #. **KRN_SCL2**: larger scale of kernel, in kpc #. **DR_LIM**: radius of matching area for the merging of detected peaks, in kpc #. **DZ_LIM**: redshift depth for the merging of detected peaks #. **FROM_DENSITY_MAP**: if True, indicates that a previously computed density map should be used as an input, therefore bypassing the first stages of PZWAV COSMOLOGY PARAMETERS KEYWORDS: #. **OMEGA_MAT**: matter energy density #. **OMEGA_VAC**: vacuum energy density #. **HUBBLE_PAR**: Hubble constant in km/s/(Mpc/h) #. **W_EQ_STATE**: dark energy equation of state #. **N_EFF**: effective number of relativistic species #. **TEMP_CMB**: CMB temperature Note : Currently, a flat LCDM model is assumed, depending only on HUBBLE_PAR and OMEGA_MAT. The list above allows a broader choice for the cosmological model (wCDM). KEYWORDS FOR RICH-CL TO MOVE TO THE CCP PIPELINE: #. **MAX_NB**: Maximum number of structures to which a galaxy can be associated #. **MIN_PROB**: Minimum probability for the association to be saved .. DetailedDescEnd