HEASoft and XSPEC are now available as conda packages. See details ....
NS Atmosphere models
Neutron star model spectra (angle-averaged surface flux) from Gaensicke, Braje & Romani 2002.
Grids for three compositions can be downloaded : hydrogen (hyd), solar (sol), iron (fe)
Each grid contains 29 spectra, covering log(Teff)=5.1 to log(Teff)=6.5 in steps of log(Teff)=0.05
The models are computed for a canonical neutron star, Mns=1.4Msun, Rns=10km, resulting in a surface gravity log g=14.386 and a redshift z=0.306.
For models with different surface gravities, or for the full angle-dependent intensities, please contact the authors.
Use the grids to fit X-ray data in XSPEC as follows:
XSPEC>model phabs(atable{fe_spectra.mod})
Model: phabs[1]( nsspec[2] )
Input parameter value, delta, min, bot, top, and max values for ...
Current: 1 0.001 0 0 1E+05 1E+06
phabs:nH>0.01
Current: 0.05 0.001 0.0108 0.0108 0.272 0.272
nsspec:kT (keV)>0.1
Current: 0 -0.001 0 0 5 5
nsspec:Redshift>0.306
Current: 1 0.01 0 0 1E+24 1E+24
nsspec:norm>1.0
XSPEC>renorm
XSPEC>fit
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Variances and Principal axes :
1 2 4
1.06E-11 | -0.03 0.06 1.00
3.16E-07 | 0.72 0.70 -0.02
7.07E-06 | 0.70 -0.71 0.06
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Model: phabs[1]( nsspec[2] )
Model Fit Model Component Parameter Unit Value
par par comp
1 1 1 phabs nH 10^22 1.5880E-02 +/- 0.1899E-02
2 2 2 nsspec kT (keV) 4.9042E-02 +/- 0.1939E-02
3 3 2 nsspec Redshift 0.3060 frozen
4 4 2 nsspec norm 2.0179E-04 +/- 0.1537E-03
Files being used for table models:
Model comp File
2 fe_spectra.mod
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Chi-Squared = 136.0014 using 81 PHA bins.
Reduced chi-squared = 1.743607 for 78 degrees of freedom
Null hypothesis probability = 5.299E-05
The distance is computed from the normalization as follows:
d[pc] = 1 / sqrt(norm) (70pc for the example above)
Please note that the original instructions on these pages contained an erroneous 1/(1+z) in the equation above. If you used these models, please check that you computed the distance with the correct relation.