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| author | Aaron LI <aaronly.me@outlook.com> | 2017-02-17 00:14:45 +0800 |
|---|---|---|
| committer | Aaron LI <aaronly.me@outlook.com> | 2017-02-17 01:16:47 +0800 |
| commit | bdc9269dcd4c5a086def4ce904528b96a475af9f (patch) | |
| tree | 9002d99d28465e1fc06e14a85334aa56a1e1e4db /mass_profile | |
| parent | a2c996d79c2bc3e854c991676680a64bd6e3195f (diff) | |
| download | chandra-acis-analysis-bdc9269dcd4c5a086def4ce904528b96a475af9f.tar.bz2 | |
Update description & usage; change variable name to be more clear
Diffstat (limited to 'mass_profile')
| -rw-r--r-- | mass_profile/calc_lx_beta.cpp | 23 | ||||
| -rw-r--r-- | mass_profile/calc_lx_dbeta.cpp | 24 |
2 files changed, 24 insertions, 23 deletions
diff --git a/mass_profile/calc_lx_beta.cpp b/mass_profile/calc_lx_beta.cpp index dcbf1ad..11d7b04 100644 --- a/mass_profile/calc_lx_beta.cpp +++ b/mass_profile/calc_lx_beta.cpp @@ -1,9 +1,10 @@ -/* - Perform a double-beta density model fitting to the surface brightness data - Author: Junhua Gu - Last modified: 2011.01.01 - This code is distributed with no warrant -*/ +/** + * Calculate the total luminosity and flux within the specified radius. + * + * Base on 'fit_beta_sbp.cpp' and supersede 'calc_lx.cpp' + * + * Author: Junhua Gu + */ #include <iostream> #include <fstream> @@ -71,7 +72,7 @@ int main(int argc,char* argv[]) { if(argc<4) { - cerr<<argv[0]<<" <configure file> <rout in kpc> <bolo erg cfunc file>"<<endl; + cerr<<argv[0]<<" <sbp.conf> <rout_kpc> <cfunc_erg> [cfunc2_erg ...]"<<endl; return -1; } //initialize the parameters list @@ -460,7 +461,7 @@ int main(int argc,char* argv[]) for(int n=3;n<argc;++n) { - spline_func_obj cf_bolo_erg; + spline_func_obj cf_erg; for(ifstream ifs(argv[n]);;) { assert(ifs.is_open()); @@ -472,12 +473,12 @@ int main(int argc,char* argv[]) } //cerr<<x<<"\t"<<y<<endl; - cf_bolo_erg.add_point(x,y);//change with source + cf_erg.add_point(x,y);//change with source } - cf_bolo_erg.gen_spline(); + cf_erg.gen_spline(); projector<double>& pj=dynamic_cast<projector<double>&>(f.get_model()); - pj.attach_cfunc(cf_bolo_erg); + pj.attach_cfunc(cf_erg); diff --git a/mass_profile/calc_lx_dbeta.cpp b/mass_profile/calc_lx_dbeta.cpp index c2f6a10..31addeb 100644 --- a/mass_profile/calc_lx_dbeta.cpp +++ b/mass_profile/calc_lx_dbeta.cpp @@ -1,10 +1,10 @@ -/* - Perform a double-beta density model fitting to the surface brightness data - Author: Junhua Gu - Last modified: 2011.01.01 - This code is distributed with no warrant -*/ - +/** + * Calculate the total luminosity and flux within the specified radius. + * + * Base on 'fit_dbeta_sbp.cpp' and supersede 'calc_lx.cpp' + * + * Author: Junhua Gu + */ #include <iostream> #include <fstream> @@ -71,7 +71,7 @@ int main(int argc,char* argv[]) { if(argc<4) { - cerr<<argv[0]<<" <configure file> <rout in kpc> <bolo erg cfunc file> "<<endl; + cerr<<argv[0]<<" <sbp.conf> <rout_kpc> <cfunc_erg> [cfunc2_erg ...]"<<endl; return -1; } //initialize the parameters list @@ -514,7 +514,7 @@ int main(int argc,char* argv[]) cout<<"dl="<<Dl/kpc<<endl; for(int n=3;n<argc;++n) { - spline_func_obj cf_bolo_erg; + spline_func_obj cf_erg; for(ifstream ifs(argv[n]);;) { assert(ifs.is_open()); @@ -526,12 +526,12 @@ int main(int argc,char* argv[]) } //cerr<<x<<"\t"<<y<<endl; - cf_bolo_erg.add_point(x,y);//change with source + cf_erg.add_point(x,y);//change with source } - cf_bolo_erg.gen_spline(); + cf_erg.gen_spline(); projector<double>& pj=dynamic_cast<projector<double>&>(f.get_model()); - pj.attach_cfunc(cf_bolo_erg); + pj.attach_cfunc(cf_erg); mv=f.eval_model_raw(radii,p); double flux_erg=0; |