Description of the algorithms used by IPP full force stage

Inputs

The Sky Calibration stage of stack photometry takes the cmf files for stack skycell and calibrates the zero point.

The current version of the IPP produces a new fits table called a cff file is created containing the parameters to be used for forced photometry for each object. (The cmf files are not used directly because they are vastly larger and would cause a much higher I/O load.

This table has one row for each source with the following columns extracted from the cmf file.

Column	Value for Extended Source	Value for Extended Source
ID	IPP_IDET	IPP_IDET
X	X_PSF	X_EXT
Y	Y_PSF	Y_EXT
FLUX	PSF_INST_FLUX/EXPTIME	10**(-0.4*EXT_INST_MAG)
AP_RADIUS	AP_MAG_RADIUS	AP_MAG_RADIUS
KRON_RADIUS	MOMENTS_R1*2.5	MOMENTS_R1*2.5
PETRO_RADIUS	PETRO_RADIUS	PETRO_RADIUS
FIT_GALAXY	0	1
PSF_STAR	PM_SOURCE_MODE_PSFSTAR	PM_SOURCE_MODE_PSFSTAR
R_MAJOR	0	EXT_WIDTH_MAJ
R_MINOR	0	EXT_WIDTH_MIN
THETA	0	EXT_THETA
MODEL_TYPE	-1	model type for best fit
INDEX	0	0.5 / EXT_PAR_07

For sources with extended fits, the FIT_GALAXY column is set and parameters from the model with the lowest EXT_CHISQ is chosen.

Full Force Run

A full force run consists of a cff file from a skycal run and the single frame warped images for the input stack's skycell filter combination. First the warps are processed by psphotFullForce and once they are all complete psphotFullForceSummary "summarizes" the results.

psphotFullForce

psphotFullForce is run separately for each input warp. Source detection is not performed, the source positions are given by the input cff file. The following psphot modules are invoked

• Model Background
• Subtract Background
• Load External Sources (read cff file)
• Full Force Stats - Construct sources and measurement moments and other basic stats on the supplied sources.
• Choose PSF
• Guess Models (only generates psf models)
• Fit Sources Linear - linear PSF fit to source peaks, subtract the models from the image (in PSF mask)
• Kron Flux - using supplied kron radius
• Petro Flux - using supplied petrosian radius
• Radial Apertures
• Galaxy Shape

The output of this process is a standard IPP cff file with an additional extension called 'XGAL' which contains the results of the galaxy shape measurements

Galaxy Shape

The galaxy shape function takes the extended fit model parameters and creates a set of models with a range of major and model radii around the input values. For each trial the model is created and the chi-squared of the model versus the warp pixels is calculated. The results of this process are saved in the XGAL extension.

psphotFullForceSummary