HEASoft and XSPEC are now available as conda packages. See details ....
Emitted spectra from a nonmagnetic carbon atmosphere of a neutron star.
This model is now in the Xspec release and this page is superceded by the Xspec manual
The fitting parameters of the model are listed below:
par1 = Effective temperature T (MK)
par2 = Neutron star mass M (M_sol)
par3 = Neutron star radius R (km)
par4 = Normalization K = A/(d_10kpc)^2
where d_10kpc is the distance to the source in units of 10 kpc and A characterizes the fraction of the star surface emitting the radiation (A=1 corresponds to the case when the radiation is emitted from the entire surface).
To use the model do the following steps:
1) extract carbatm.tar.gz, which will create a directory named "carbatm" containing all necessary files. To compile and to use the model, a writing access to the directory is necessary!
2) to compile the model, launch XSPEC 12 and execute the following command XSPEC12> initpackage mypackage model.dat /full-path-to-carbatm/carbatm/
3) load the compiled model package with "lmod" command: XSPEC12> lmod mypackage /full-path-to-carbatm/carbatm/
4) Copy the directory carbatm/catm_tables to $HEADAS/../spectral/modelData/ or, alternatively, use the "xset" command of XSPEC to set the CARBATM variable to the full path to the directory containing the "catm_tables" subdirectory:
XSPEC12> xset CARBATM /full-path-to/carbatm/ (Note: /full-path-to/carbatm/ should *not* include the "catm_tables" itself).
The model is now available under the name "carbatm".
Please send any questions and comments to suleimanov@astro.uni-tuebingen.de or klochkov@astro.uni-tuebingen.de