BHSPEC
BHSPEC
is an additive table model for use with the
Xspec spectral
fitting package.
It is comprised of a tabulation of artificial SEDs for disks accreting
onto black holes. These SEDs were computed using the TLUSTY stellar atmospheres
code.
- Original Xspec table models:
These table files were the first to be publicly released and are available via
the Xspec website.
bhspec.fits
covers a spin (a/M) range from 0 to 0.8 for alpha 0.01 and 0.1.
bhspec2.fits
covers a larger range in spins (a/M from 0 to 0.99) but is
tabulated only for alpha=0.01.
- New Xspec table models:
These table files are identical to the originals (above), but cover a wider
range of parameter space in spin and mass.
bhspec_spin_0.1.fits
covers an extended spin (a/M) range from -1.0 to 0.8 for alpha=0.1 (log L/L_Edd from -2 to 0).
bhspec_spin2_0.1.fits
covers an extended spin (a/M) range from 0 to 0.99 for alpha=0.1 (log L/L_Edd from -1.5 to -0.5).
bhspec_spin_0.01.fits
covers an extended spin (a/M) range from -1.0 to 0.99 for alpha=0.01.
bhspec_mass_0.1.fits
covers an extended mass range from 3 to 300 solar masses for alpha=0.1.
bhspec_mass_0.01.fits
covers an extended mass range from 3 to 300 solar masses for alpha=0.01.
bhspec_mean_0.1.fits
mean stress prescription with alpha=0.1. See Done & Davis, 2008, ApJ, 683, 389 for description.
The next two models cover a lower mass range (M=1-2 solar masses), but are
otherwise identical to those above (i.e. Kerr spacetime). Note that the mass
variable for these models is simply mass rather than log(mass), as it is in the
above models.
bhspec_lowmass_0.01.fits
covers log L/L_Edd from -2 to 0 and a/M from 0 to 0.5 for alpha=0.01
bhspec_lowmass_0.1.fits
covers log L/L_Edd from -1.7 to 0 and a/M from 0 to 0.5 for alpha=0.1
- Brief summary of the BHSPEC model:
bhspec.ps
bhspec.pdf
-
If these models are used for published research, Davis & Hubeny (2006) should be cited:
"A Grid of Relativistic, non-LTE Accretion Disk Models for Spectral Fitting of Black Hole
Binaries"
Davis, S. W. & Hubeny, I. 2006, ApJS, 164, 530
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-
A selection of publications which utilize these models:
McClintock et al., 2006:
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Middleton et al., 2006:
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Shafee et al., 2006:
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Davis et al. 2006:
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- A selection of other related publications:
Blaes et al. 2006:
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Davis et al. 2005:
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Hubeny et al. 2001:
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Hubeny & Hubeny 1998:
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Agol 1997:
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Hubeny & Lanz 1995:
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- Annuli Spectra Used to Generate the BHSPEC Model:
annuli.tar.gz
A brief description of the annuli spectra:
annuli.ps