XSlaor¶
-
class
sherpa.astro.xspec.
XSlaor
(name='laor')[source] [edit on github]¶ Bases:
sherpa.astro.xspec.XSAdditiveModel
The XSPEC laor model: accretion disk, black hole emission line.
The model is described at 1.
Note
Deprecated in Sherpa 4.10.0
The
RinG
andRoutG
parameters have been renamed toRin_G
andRout_G
respectively to match the XSPEC definition. The namesRinG
andRoutG
can still be used to access the parameters, but they will be removed in a future release.-
lineE
¶ The rest-frame line energy, in keV.
-
Index
¶ The power law dependence of emissivity (scales as R^-Index).
-
Rin_G
¶ The inner radius, in units of GM/c^2.
-
Rout_G
¶ The outer radius, in units of GM/c^2.
-
Incl
¶ The disk inclination angle, in degrees. A face-on disk has Incl=0.
-
norm
¶ The flux in the line, in units of photon/cm^2/s.
References
Attributes Summary
The hard maximum values for the thawed parameters.
The hard minimum values for the thawed parameters.
Access to the maximum limits for the thawed parameters
Access to the minimum limits for the thawed parameters
Access to the thawed parameters of the model
Methods Summary
apply
(outer, *otherargs, **otherkwargs)calc
(pars, xlo, *args, **kwargs)Evaluate the model on a grid.
guess
(dep, *args, **kwargs)Set an initial guess for the parameter values.
regrid
(*args, **kwargs)The class RegriddableModel1D allows the user to evaluate in the requested space then interpolate onto the data space.
reset
()Reset the parameter values.
set_center
(*args, **kwargs)startup
([cache])Called before a model may be evaluated multiple times.
teardown
()Called after a model may be evaluated multiple times.
Attributes Documentation
-
ndim
= 1¶
-
thawedparhardmaxes
¶ The hard maximum values for the thawed parameters.
-
thawedparhardmins
¶ The hard minimum values for the thawed parameters.
-
thawedparmaxes
¶ Access to the maximum limits for the thawed parameters
-
thawedparmins
¶ Access to the minimum limits for the thawed parameters
-
thawedpars
¶ Access to the thawed parameters of the model
-
version_enabled
= True¶
Methods Documentation
-
apply
(outer, *otherargs, **otherkwargs) [edit on github]¶
-
calc
(pars, xlo, *args, **kwargs) [edit on github]¶ Evaluate the model on a grid.
- Parameters
p (sequence of numbers) – The parameter values to use. The order matches the
pars
field.*args – The model grid. The values can be scalar or arrays, and the number depends on the dimensionality of the model and whether it is being evaluated over an integrated grid or at a point (or points).
-
get_center
() [edit on github]¶
-
guess
(dep, *args, **kwargs)[source] [edit on github]¶ Set an initial guess for the parameter values.
Attempt to set the parameter values, and ranges, for the model to match the data values. This is intended as a rough guess, so it is expected that the model is only evaluated a small number of times, if at all.
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regrid
(*args, **kwargs) [edit on github]¶ The class RegriddableModel1D allows the user to evaluate in the requested space then interpolate onto the data space. An optional argument ‘interp’ enables the user to change the interpolation method.
Examples
>>> import numpy as np >>> from sherpa.models.basic import Box1D >>> mybox = Box1D() >>> request_space = np.arange(1, 10, 0.1) >>> regrid_model = mybox.regrid(request_space, interp=linear_interp)
-
reset
() [edit on github]¶ Reset the parameter values.
-
set_center
(*args, **kwargs) [edit on github]¶
-
startup
(cache=False) [edit on github]¶ Called before a model may be evaluated multiple times.
- Parameters
cache (bool, optional) – Should a cache be used when evaluating the models.
See also
-
teardown
() [edit on github]¶ Called after a model may be evaluated multiple times.
See also
setup()
-