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e_lensing.c
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Sun, Dec 29, 08:49

e_lensing.c
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#include<stdio.h>
#include<math.h>
#include<fonction.h>
#include<constant.h>
#include<dimension.h>
#include<structure.h>
/****************************************************************/
/* nom: e_lensing */
/* auteur: Jean-Paul Kneib */
/* date: 10/02/92 */
/* place: Toulouse */
/****************************************************************
* For each source of the source list, find the list of corresponding
* arclets and apply a special treatment to those with a tau parameter
* larger than large_dist.
*
* The correspondance between the source and the image planes required
* that the gimage grid is initialized.
*
* Parameters :
* - source : a list of sources
* - image[nb_familly][nb_arclets] : a list of arclets
*
* Calling sequence : e_lensing() -> e_lens() -> e-test() -> e_mag() -> diag()
*/
void e_lensing( struct galaxie source[NFMAX],
struct galaxie image[NFMAX][NIMAX] )
{
extern struct g_mode M;
const extern struct g_source S;
const extern struct g_large L;
extern struct point gsource_global[NGGMAX][NGGMAX];
long int i;
double dlsds;
int ngiant;
long int ni, nfound, nmissed;
int save;
dlsds = 0;
ngiant = ni = nfound = nmissed = 0;
/* classement des sources par z croissant if the sources have different z*/
i = 1;
while ( i < S.ns && source[i].z == source[i-1].z ) i++;
if ( i < S.ns )
sort(S.ns, source, comparer_z);
// Switch to silent mode if we create a weak-lensing catalog
save = M.verbose;
if ( M.image == 0 && M.source == 0 )
M.verbose = -1;
// Initialize the image array
for ( i = 0 ; i < S.ns ; i++ )
{
/*if the source is behind the cluster */
if ( source[i].dr > PREC_DLSDS )
{
/*initialize the gsource grid for the source i*/
if ( source[i].dr != dlsds )
{
dlsds = source[i].dr;
NPRINTF(stderr, "COMP: grid at z=%.3lf (%.3lf)\n", source[i].z, dlsds);
e_unlensgrid(gsource_global, dlsds);
}
/*find the arclets corresponding to source[i] and fill the
* image[familly][arclets] list*/
if ( M.verbose == -1 )
fprintf( stderr, "Compute multiple images for source %ld...", i);
ni = e_lens( source[i] , image[i] );
nfound += ni;
if ( ni == 0 ) nmissed++;
if ( M.verbose == -1 )
fprintf( stderr, "images found %ld, not found %ld\r", nfound, nmissed);
/*fill the tau parameter of the arclets*/
e_tau(ni, image[i]);
sort(ni, image[i], comparer_tau);
if ( image[i][0].tau > L.dlarge || L.dlarge < 0.1 )
e_giant( &ngiant, source[i], image[i] );
}
}
if ( nmissed != 0 )
fprintf( stderr, "\nWARN: There were missed images probably due to the grid resolution.\n");
M.verbose = save;
if ( ngiant != 0 )
w_gianti( ngiant , "gianti.dat" );
}

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