Detection Parameters Input Product for¶
Data product name¶
detclParameters
Data product custodian¶
DET-CL
Data model tag¶
DpdLE3clCcpInputParams
Name of the Schema file¶
test-le3-cl-ccp-params.xsd
Schema documentation tag¶
This product contains the input parameters for DET-CL
Data product elements¶
- Header
type sys:genericHeader
- Data
type cl:ccpParametersList
- QualityFlags
type dqc:sqfPlaceHolder
- Parameters
type ppr:genericKeyValueParameters
Processing Element(s) creating/using the data product¶
DET-CL
Processing function using the data product¶
LE3, “DET-CL” pipeline
Detailed description of the data product¶
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