XSdiskline

class sherpa.astro.xspec.XSdiskline(name='diskline')

Bases: sherpa.astro.xspec.XSAdditiveModel

The XSPEC diskline model: accretion disk line emission, relativistic.

The model is described at [1].

Note

Deprecated in Sherpa 4.10.0

The RinM and RoutM parameters have been renamed Rin_M and Rout_M respectively to match the XSPEC definition. The names RinM and RoutM can still be used to access the parameters, but they will be removed in a future release.

LineE

The line energy in keV.

Betor10

The power law dependence of emissivity: see [1] for more details.

Rin_M

The inner radius, in units of GM^2/c.

Rout_M

The outer radius, in units of GM^2/c.

Incl

The inclination, in degrees.

norm

The model normalization in photon/cm^2/s.

References

[1]	(1, 2) https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelDiskline.html

Attributes Summary

thawedparhardmaxes
thawedparhardmins
thawedparmaxes
thawedparmins
thawedpars
version_enabled

Methods Summary

apply(outer, \*otherargs, \*\*otherkwargs)
calc(pars, xlo, \*args, \*\*kwargs)
get_center()
guess(dep, \*args, \*\*kwargs)
reset()
set_center(\*args, \*\*kwargs)
startup()
teardown()

Attributes Documentation

thawedparhardmaxes

thawedparhardmins

thawedparmaxes

thawedparmins

thawedpars

version_enabled = True

Methods Documentation

apply(outer, *otherargs, **otherkwargs)

calc(pars, xlo, *args, **kwargs)

get_center()

guess(dep, *args, **kwargs)

reset()

set_center(*args, **kwargs)

startup()

teardown()