1 files changed, 0 insertions, 140 deletions
diff --git a/astro/cosmo_calc/main.cc b/astro/cosmo_calc/main.cc
deleted file mode 100644
index bbd73ba..0000000
--- a/astro/cosmo_calc/main.cc
+++ /dev/null
@@ -1,140 +0,0 @@
-//
-// simple `cosmology calculator'
-// can calc commonly used cosmology distances:
-//      hubble distance
-//      comoving distance
-//      transverse comoving distance
-//      angular diameter distance
-//      luminoisity distance
-//      light-travel distance
-// in addition, this calculator also calc some other
-// useful infomation related with Chandra
-//
-// Junhua Gu
-//
-// Modified by: LIweitiaNux
-//
-// ChangeLogs:
-// v2.1, 2012/08/12, LIweitiaNux
-//   improve cmdline parameters
-// v2.2, 2013/02/09, LIweitiaNux
-//   add 'hubble_parameter E(z)'
-//   modify output format
-//
-
-
-#include "calc_distance.h"
-#include "ddivid.h"
-#include <cstdio>
-#include <cstdlib>
-#include <cmath>
-#include <iostream>
-
-using namespace std;
-
-// extern variables in `calc_distance.h'
-extern double cm;
-extern double s;
-extern double km;
-extern double Mpc;
-extern double kpc;
-extern double yr;
-extern double Gyr;
-extern double H0;           // units: [km/s/Mpc]
-extern double c;
-extern double omega_m;
-extern double omega_l;
-extern double omega_k;
-extern double arcsec2arc_ratio;
-
-// README, ABOUT
-static char DESC[] = "simple cosmology calculator";
-static char VER[]  = "v2.2, 2013-02-09";
-
-// setting parameters
-static double PI = 4*atan(1.0);
-// chandra related
-static double arcsec_per_pixel = 0.492;
-// above cosmology paramters can also be changed
-// through cmdline paramters
-
-// functions
-void usage(const char *name);
-
-//////////////////////////////////////////////
-// main part
-//////////////////////////////////////////////
-int main(int argc,char* argv[])
-{
-    double z;       // given redshift
-
-    // cmdline parameters
-    if (argc == 2) {
-        // get input redshift
-        z = atof(argv[1]);
-    }
-    else if (argc == 3) {
-        z = atof(argv[1]);
-        // use specified `H0'
-        H0 = atof(argv[2]);
-    }
-    else if (argc == 4) {
-        z = atof(argv[1]);
-        H0 = atof(argv[2]);
-        // get specified `Omega_M'
-        omega_m = atof(argv[3]);
-        omega_l = 1.0-omega_m;
-    }
-    else {
-        usage(argv[0]);
-        exit(-1);
-    }
-
-    // calc `Hubble parameter E(z)'
-    double E_z = E(z);
-    // calc `comoving distance'
-    double d_C = calc_comoving_distance(z);
-    // calc `angular diameter distance'
-    double d_A = calc_angdia_distance(z);
-    // calc `luminoisity distance'
-    double d_L = calc_luminosity_distance(z);
-
-    // output results
-    // parameters
-    printf("Parameters:\n");
-    printf("  z= %lf, H0= %lf, Omega_M= %lf, Omega_L= %lf\n",
-            z, H0, omega_m, omega_l);
-    printf("Distances:\n");
-    printf("  Comoving_distance: D_C(%lf)= %lg [cm], %lf [Mpc]\n",
-            z, d_C, d_C/Mpc);
-    printf("  Angular_diameter_distance: D_A(%lf)= %lg [cm], %lf [Mpc]\n",
-            z, d_A, d_A/Mpc);
-    printf("  Luminoisity_distance: D_L(%lf)= %lg [cm], %lf [Mpc]\n",
-            z, d_L, d_L/Mpc);
-    printf("Chandra_related:\n");
-    printf("  kpc/pixel (D_A): %lf\n",
-            (d_A / kpc * arcsec_per_pixel* arcsec2arc_ratio));
-    printf("  cm/pixel (D_A): %lg\n",
-            (d_A * arcsec_per_pixel* arcsec2arc_ratio));
-    printf("Other_data:\n");
-    printf("  Hubble_parameter: E(%lf)= %lf\n", z, E_z);
-    printf("  kpc/arcsec (D_A): %lf\n", (d_A / kpc * arcsec2arc_ratio));
-    printf("  norm (cooling_function): %lg\n",
-            (1e-14 / (4.0 * PI * pow(d_A*(1+z), 2))));
-
-    //cout<<ddivid(calc_distance,d,0,1,.0001)<<endl;
-
-    return 0;
-}
-
-// other auxiliary functions
-void usage(const char *name)
-{
-    cerr << "Usage: " << endl;
-    cerr << "    " << name << " z [H0] [Omega_M]" << endl;
-    // description
-    cout << endl << "About:" << endl;
-    cout << DESC << endl << VER << endl;
-}
-
-/* vim: set ts=8 sw=4 tw=0 fenc=utf-8 ft=cpp: */