Beispiel #1
0
int main(int argc, char *argv[]){

  SID_init(&argc,&argv,NULL,NULL);

  char   filename_cosmology[MAX_FILENAME_LENGTH];
  char   paramterization[MAX_FILENAME_LENGTH];
  double log_M_min    =atof(argv[1]);
  double log_M_max    =atof(argv[2]);
  int    n_M_bins     =atoi(argv[3]);
  double redshift     =atof(argv[4]);
  strcpy(filename_cosmology,argv[5]);
  strcpy(paramterization,   argv[6]);

  SID_log("Constructing mass function between log(M)=%5.3lf->%5.3lf at z=%5.3lf...",SID_LOG_OPEN,log_M_min,log_M_max,redshift);

  // Initialize cosmology
  cosmo_info *cosmo=NULL;
  read_gbpCosmo_file(&cosmo,filename_cosmology);

  // Decide which parameterization we are going to use
  int  select_flag;
  char mfn_text[32];
  if(!strcmp(paramterization,"JENKINS")){
     sprintf(mfn_text,"Jenkins");
     select_flag=MF_JENKINS;
  }
  else if(!strcmp(paramterization,"PS")){
     sprintf(mfn_text,"Press & Schechter");
     select_flag=MF_PS;
  }
  else if(!strcmp(paramterization,"ST")){
     sprintf(mfn_text,"Sheth & Tormen");
     select_flag=MF_ST;
  }
  else
     SID_trap_error("Invalid parameterization selected {%s}.  Should be {JENKINS,PS or ST}.",ERROR_SYNTAX,paramterization);

  // Create output filename
  char  filename_out[MAX_FILENAME_LENGTH];
  char  redshift_text[64];
  char *cosmology_name=(char *)ADaPS_fetch(cosmo,"name");
  float_to_text(redshift,3,redshift_text);
  sprintf(filename_out,"mass_function_z%s_%s_%s.txt",redshift_text,cosmology_name,paramterization);

  // Open file and write header
  FILE *fp_out=NULL;
  fp_out=fopen(filename_out,"w");
  int i_column=1;
  fprintf(fp_out,"# Mass function (%s) for %s cosmology at z=%lf\n",mfn_text,filename_cosmology,redshift);
  fprintf(fp_out,"# \n");
  fprintf(fp_out,"# Column (%02d): log M [h^-1 M_sol]\n",                              i_column++);
  fprintf(fp_out,"#        (%02d): Mass function [(h^{-1} Mpc]^{-3} per dlogM]\n",     i_column++);
  fprintf(fp_out,"#        (%02d): Cumulative Mass function(>M) [(h^{-1} Mpc]^{-3}]\n",i_column++);

  // Create the mass function
  SID_log("Writing results to {%s}...",SID_LOG_OPEN|SID_LOG_TIMER,filename_out);
  pcounter_info pcounter;
  SID_init_pcounter(&pcounter,n_M_bins,10);
  double h_Hubble   =((double *)ADaPS_fetch(cosmo,"h_Hubble"))[0];
  double mass_factor=M_SOL/h_Hubble;
  double MFct_factor=pow(M_PER_MPC,3.0);
  for(int i_bin=0;i_bin<n_M_bins;i_bin++){
     double log_M;
     if(i_bin==0)
        log_M=log_M_min;
     else if(i_bin==(n_M_bins-1))
        log_M=log_M_max;
     else
        log_M=log_M_min+(((double)(i_bin))/((double)(n_M_bins-1)))*(log_M_max-log_M_min);
     fprintf(fp_out,"%le %le %le\n",log_M,
                                    MFct_factor*mass_function           (mass_factor*take_alog10(log_M),redshift,&cosmo,select_flag),
                                    MFct_factor*mass_function_cumulative(mass_factor*take_alog10(log_M),redshift,&cosmo,select_flag));
     SID_check_pcounter(&pcounter,i_bin);
  }
  fclose(fp_out);
  SID_log("Done.",SID_LOG_CLOSE);

  // Clean-up
  free_cosmo(&cosmo);

  SID_log("Done.",SID_LOG_CLOSE);
  SID_exit(ERROR_NONE);
}
int main(int argc, char *argv[]){
   double  redshift;
   char    filename_in[MAX_FILENAME_LENGTH];
   char    filename_out[MAX_FILENAME_LENGTH];
   char    filename_cosmology[MAX_FILENAME_LENGTH];
   double  box_size;
   double  lM_min,dlM;
   char   *line=NULL;
   size_t  line_length=0;
   int     M_column;
   int     n_bins;
   int     flag_log;
 
   // Initialization -- MPI etc.
   SID_init(&argc,&argv,NULL,NULL);
   if(argc!=11)
     SID_trap_error("Incorrect syntax.",ERROR_SYNTAX);

   // Parse arguments
   strcpy(filename_in, argv[1]);
   strcpy(filename_out,argv[2]);
   redshift=(double)atof(argv[3]);
   strcpy(filename_cosmology,argv[4]);
   box_size=(double)atof(argv[5]);
   M_column=(int)   atoi(argv[6]);
   flag_log=(int)   atoi(argv[7]);
   lM_min  =(double)atof(argv[8]);
   dlM     =(double)atof(argv[9]);
   n_bins  =(int)   atoi(argv[10]);

   SID_log("Producing a mass function for ascii file {%s}...",SID_LOG_OPEN|SID_LOG_TIMER,filename_in);
 
   // Initialize cosmology
   cosmo_info *cosmo;
   read_gbpCosmo_file(&cosmo,filename_cosmology);
   double h_Hubble=((double *)ADaPS_fetch(cosmo,"h_Hubble"))[0];

   // Open file
   FILE *fp_in;
   if((fp_in=fopen(filename_in,"r"))==NULL)
      SID_trap_error("Could not open {%s} for reading.",ERROR_IO_OPEN,filename_in);

   // Allocate memory for the data. Read it and sort it in ascending order 
   SID_log("Reading data...",SID_LOG_OPEN|SID_LOG_TIMER);
   int     n_data_in=count_lines_data(fp_in);
   SID_log("(%d items)...",SID_LOG_CONTINUE,n_data_in);
   double *data  =(double *)malloc(sizeof(double)*n_data_in);
   int n_data=0;
   for(int i=0;i<n_data_in;i++){
     double data_in;
     grab_next_line_data(fp_in,&line,&line_length);
     grab_double(line,M_column,&data_in);
     if(!flag_log)
        data_in=take_log10(data_in);
     if(data_in>=lM_min)
        data[n_data++]=data_in;
   }
   SID_log("(%d will be used)...",SID_LOG_CONTINUE,n_data);
   fclose(fp_in);
   SID_free(SID_FARG line);
   SID_log("Done.",SID_LOG_CLOSE);

   // Perform sort
   SID_log("Sorting data...",SID_LOG_OPEN|SID_LOG_TIMER);
   merge_sort(data,n_data,NULL,SID_DOUBLE,SORT_INPLACE_ONLY,SORT_COMPUTE_INPLACE);
   SID_log("Done.",SID_LOG_CLOSE);

   // Compile histogram
   SID_log("Computing mass function...",SID_LOG_OPEN|SID_LOG_TIMER);
   double *bin       =(double *)SID_malloc(sizeof(double)*(n_bins+1));
   double *bin_median=(double *)SID_malloc(sizeof(double)*n_bins);
   int    *hist      =(int    *)SID_calloc(sizeof(int)   *n_bins);
   double  lM_bin_min=lM_min;
   double  lM_bin_max=lM_min;
   int     i_data_lo=-1;
   int     i_data_hi=-1;
   int     i_bin =0;
   int     i_data=0;
   for(i_bin=0;i_bin<n_bins;i_bin++){
     lM_bin_min=lM_bin_max;
     lM_bin_max=lM_min+((double)(i_bin+1))*dlM;
     bin[i_bin]=lM_bin_min;
     i_data_lo=i_data;
     i_data_hi=i_data;
     while(data[i_data]<lM_bin_max && i_data<n_data){
        hist[i_bin]++;
        i_data_hi=i_data;
        i_data++;
        if(i_data>=n_data) break;
     }
     int i_data_mid=(i_data_lo+i_data_hi)/2;
     if(hist[i_bin]>0){
       if(hist[i_bin]%2)
         bin_median[i_bin]=data[i_data_mid];
       else
         bin_median[i_bin]=0.5*(data[i_data_mid]+data[i_data_mid+1]);
     }
     else
        bin_median[i_bin]=0.5*(lM_bin_max+lM_bin_min);
   }
   bin[i_bin]=lM_bin_max;
   SID_log("Done.",SID_LOG_CLOSE);

   // Write mass function
   FILE *fp_out;
   if((fp_out=fopen(filename_out,"w"))==NULL){
     fprintf(stderr,"Error opening output file {%s}.\n",filename_out);
     SID_free(SID_FARG data);
     return(1);
   }
   SID_log("Writing results to {%s}...",SID_LOG_OPEN|SID_LOG_TIMER,filename_out);
   double box_volume=box_size*box_size*box_size;
   fprintf(fp_out,"# Mass function for column %d in {%s}\n",M_column,filename_in);
   fprintf(fp_out,"# Column (01): M_lo     [source units]\n");
   fprintf(fp_out,"#        (02): M_median [source units]\n");
   fprintf(fp_out,"#        (03): M_hi     [source units]\n");
   fprintf(fp_out,"#        (04): No. in bin\n");
   fprintf(fp_out,"#        (05): MFn (per unit volume, per dlogM)\n");
   fprintf(fp_out,"#        (06): +/- MFn\n");
   fprintf(fp_out,"#        (07): Sheth & Tormen MFn\n");
   fprintf(fp_out,"#        (08): Watson MFn\n");
   fprintf(fp_out,"#        (09): No. w/ M>M_lo\n");
   fprintf(fp_out,"#        (10): Cumulative MFn (per unit volume)\n");
   fprintf(fp_out,"#        (11): +/- Cumulative MFn\n");
   fprintf(fp_out,"#        (12): Sheth & Tormen Cumulative MFn\n");
   fprintf(fp_out,"#        (13): Watson Cumulative MFn\n");
   double M_sol_inv_h=M_SOL/h_Hubble;
   double Mpc_inv_h  =M_PER_MPC/h_Hubble;
   for(int i=0;i<n_bins;i++){
     double dn_dlogM_theory_1=mass_function(take_alog10(bin_median[i])*M_sol_inv_h,
                                            redshift,
                                            &cosmo,
                                            MF_ST)*pow(Mpc_inv_h,3.0);
     double n_theory_1=mass_function_cumulative(take_alog10(bin[i])*M_sol_inv_h,
                                                redshift,
                                                &cosmo,
                                                MF_ST)*pow(Mpc_inv_h,3.0);
     double dn_dlogM_theory_2=mass_function(take_alog10(bin_median[i])*M_sol_inv_h,
                                            redshift,
                                            &cosmo,
                                            MF_WATSON)*pow(Mpc_inv_h,3.0);
     double n_theory_2=mass_function_cumulative(take_alog10(bin[i])*M_sol_inv_h,
                                                redshift,
                                                &cosmo,
                                                MF_WATSON)*pow(Mpc_inv_h,3.0);
     // Compute cumulative histogram
     int cumulative_hist=0;
     for(int j_bin=i;j_bin<n_bins;j_bin++)
        cumulative_hist+=hist[j_bin];
     fprintf(fp_out,"%11.4le %11.4le %11.4le %6d %11.4le %11.4le %10.4le %10.4le %6d %10.4le %10.4le %10.4le %10.4le\n",
             bin[i],
             bin_median[i],
             bin[i+1],
             hist[i],
             (double)(hist[i])/(box_volume*dlM),
             sqrt((double)(hist[i]))/(box_volume*dlM),
             dn_dlogM_theory_1,dn_dlogM_theory_2,
             cumulative_hist,
             (double)(cumulative_hist)/box_volume,
             sqrt((double)(cumulative_hist))/box_volume,
             n_theory_1,n_theory_2);
   }
   fclose(fp_out);
   SID_log("Done.",SID_LOG_CLOSE);

   // Free allocated memory
   SID_free(SID_FARG data);
   SID_free(SID_FARG bin);
   SID_free(SID_FARG bin_median);
   SID_free(SID_FARG hist);
  
   SID_log("Done.",SID_LOG_CLOSE);
   SID_exit(ERROR_NONE);
}