Come analyze HEASARC, IRSA, and MAST data in the cloud! The Fornax Initiative is now welcoming all interested beta users.
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This model is now in the Xspec release and this page is superceded by the Xspec manual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