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r_cosmolimit.c
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Sun, Jan 5, 23:30

r_cosmolimit.c
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#include<stdio.h>
#include<string.h>
#include<math.h>
#include<fonction.h>
#include<constant.h>
#include<dimension.h>
#include<structure.h>
#include<lt.h>
/****************************************************************/
/* Program : lenstool */
/* Version : Feb 13, 2006 */
/* Location : ESO, Chile */
/* Auteur : Eric Jullo *
****************************************************************
* Read and set the limits on the cosmological parameters.
*/
void r_cosmolimit(FILE *IN, FILE *OUT)
{
extern struct g_cosmo clmin, clmax;
extern int cblock[NPAMAX];
char second[20], third[FILENAME_SIZE+10];
fmot(IN, second);
while (strcmp(second, "end"))
{
flire(IN, third);
CHECK_THIRD(FILENAME_SIZE+10)
if (!strcmp(second, "omegaM") || !strcmp(second, "omega"))
{
sscanf(third, "%d %lf %lf", &cblock[OMEGAM],
&clmin.omegaM, &clmax.omegaM);
fprintf(OUT, "\t%s\t%d %lf %lf\n", second, cblock[OMEGAM],
clmin.omegaM, clmax.omegaM);
}
else if (!strcmp(second, "omegaX") ||
!strcmp(second, "lambda") ||
!strcmp(second, "omegaL") )
{
sscanf(third, "%d %lf %lf", &cblock[OMEGAX],
&clmin.omegaX, &clmax.omegaX);
fprintf(OUT, "\t%s\t%d %lf %lf\n", second, cblock[OMEGAX],
clmin.omegaX, clmax.omegaX);
}
else if (!strcmp(second, "wX"))
{
sscanf(third, "%d %lf %lf", &cblock[WX],
&clmin.wX, &clmax.wX);
fprintf(OUT, "\t%s\t%d %lf %lf\n", second, cblock[WX],
clmin.wX, clmax.wX);
}
else if (!strcmp(second, "wa"))
{
sscanf(third, "%d %lf %lf", &cblock[WA],
&clmin.wa, &clmax.wa);
fprintf(OUT, "\t%s\t%d %lf %lf\n", second, cblock[WA],
clmin.wa, clmax.wa);
};
// Read the next line
fmot(IN, second);
}
fprintf(OUT, "\t%s\n", second);
}

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