/* MX LIBRARY FUNCTION: mxqdphot0_qdt1_vf5; * * PURPOSE: Dump the results * * AUTHOR: K. J. Mighell (mighell@noao.edu) * * LANGUAGE: ANSI C * * DOCUMENTATION: http://www.noao.edu/staff/mighell/mx * * DATE: 20000316 * * MOD: 2 * * Copyleft (L) 2000 Kenneth John Mighell */ #include #include "mxqdphot.h" void mxqdphot0_qdt1_vf5 ( double *outv, int szoutv, int nstr, FILE *out1fd, FILE *out2fd ){ char mxfunc[] = "mxqdhot0_qdt1_vf5"; int j; int index; int ok; FILE *ofd; for (j=0; j 1 electrons]\n"); fprintf (ofd, "# (6) error of stellar magnitude [mag]\n"); fprintf (ofd, "# (7) signal within stellar aperture [electrons]\n"); fprintf (ofd, "# (8) area of stellar aperture [px]\n"); fprintf (ofd, "# (9) sky value of background aperture [electrons]\n"); fprintf (ofd, "# (10) error of sky value [electrons]\n"); fprintf (ofd, "# (11) number of pixels used to estimate sky value [px]\n"); } } ok: return; } /* end-of-file */