ALGORITHM | str | Which algorithm shall be run (either AMICO, PZWAV, or BOTH) | |
AuxInfo | ClGenericContainer | Auxiliary configuration information | |
AVEPZ_MAG_DEPENDENCE | str | If true, the average P(z) is made magnitude dependent | |
AVEPZ_MIN_PZ_CONTRIB | float | Minimum P(z) value for which a galaxy is used for computing the average P(z) | |
CUBE_XY_STEP | float | Size [deg] of the Amplitude bins in the X- and Y-dimensions | |
DR_LIM | float | Radius of matching area for the merging of detected peaks, in kpc | |
DZ | float | Half width of reach redshift slice | |
DZ_LIM | float | Redshift depth for the merging of detected peaks | |
FROM_DENSITY_MAP | str | Flag indicating if a previously computed density map should be used as an input, therefore bypassing the first stages of PZWav | |
GRAY_WIDTH | float | Width in deg of the gray area | |
KRN_SCL1 | float | Lower scale of kernel, in kpc | |
KRN_SCL2 | float | Upper scale of kernel, in kpc | |
LAMBDA_STAR_THRESHOLD | float | Minimum value of lambda* for which detections are kept | |
MAX_LOST_PZ_INTEGRAL_PROB | float | Maximum galaxy P(z) lost when cutting redshift range | |
MAX_Z | float | Upper limit of redshift range for cluster detection | |
MIN_Z | float | Lower limit of redshift range for cluster detection | |
NOISE_VALUE_MIN | float | Minimum value imposed for the noise | |
NOISE_VALUE_ZEROS | float | Value assigned to all the noise pixels with values close to 0 | |
SNR_THR_AMICO | float | The S/N lower threshold for extracting a detection with AMICO | |
SNR_THR_PZWAV | float | The S/N lower threshold for extracting a detection with PZWAV | |
ZSTEP | float | Interval between slices | |