A tool that enables the user to create table and cdfp files that contain calibrated photometric parameters (i.e. aperture magnitudes and sky surface brightness values) along with astrometric positions from the image WCS (in the header).

For this code to run we must have WCS and photometric keywords properly intalled in the input image header. To check that everyting is valid for running midophot2cdfp I use the code midophotcat_prep, which will also prepare a table of astrometric positions using the routine midowcs.

% midoquery --help