Basic Usage

If the kabukinai binaries aren't in your PATH, you may need to prefix these commands by something like kabukinai/build/bin/.

To make a point spread function with default parameters:

# psfgen psf.fits

Kabukinai itself needs input in the form of a tab separated value (TSV) file. The columns are floating point numbers representing the CCD X and Y pixel coordinates and the intensities of point sources. The X and Y coordinates need not be on the CCD: kabukinai will include the "wings" of the point spread functions of stars up to 32 pixels outside the CCD bounds.

# kabukinai psf.fits star_data.tsv output.fits