NS Atmosphere modelsNeutron 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 --------------------------------------------------------------------------- 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 --------------------------------------------------------------------------- --------------------------------------------------------------------------- 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 --------------------------------------------------------------------------- --------------------------------------------------------------------------- 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.
Keith Arnaud, Lab. for High Energy Astrophysics, NASA/Goddard Space Flight Center HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public Last modified: Wednesday, 04-Jun-2003 11:35:11 EDT 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. |