HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.
Emitted spectra from a nonmagnetic carbon
atmosphere of a neutron star.
NOTE: This model is now in the Xspec release and this page is superceded by the Xspec manual
The model provides the spectra emitted from a nonmagnetic carbon
atmosphere of a neutron star. The model spectra in a 0 - 20 keV range
of (unredshifted) photon energy are computed on a grid of surface
gravity accelerations log(g) = 13.7 - 14.9 (in cgs units) and effective
temperatures T = 1 - 4 MK. For a given set of the fitting parameters,
the surface gravity g and the gravitational redshift z are derived
from the mass M and radius R of the star. The trial spectra are
computed using a linear interpolation between the nearest model
spectra on the T-log(g) grid, and the boundaries of the energy bins.
The number of photons in each bin are divided by (1+z). This is an
updated version of the models presented in
Suleimanov et al. 2014, ApJS 210, 13.
http://adsabs.harvard.edu/abs/2014ApJS..210...13S
The details can be found in Suleimanov, Klochkov et al. 2016 (A&A, submitted).
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
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Last modified: Tuesday, 14-Feb-2023 16:41:51 EST
HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.
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