Last modified: December 2018

URL: http://cxc.harvard.edu/sherpa/ahelp/models.html
AHELP for CIAO 4.11 Sherpa v1

models

Context: models

Synopsis

Summary of Sherpa models (excluding XSPEC)

Description

The following table lists most of the models available within Sherpa. See "ahelp xs" for those models provided by XSPEC, and "ahelp tablemodel" and "ahelp load_user_model" for information on table and user-supplied models, respectively.

Sherpa models (exclding those from XSPEC)

Model name Description
absorptionedge Optical model of an absorption edge.
absorptiongaussian Gaussian function for modeling absorption (equivalent width).
absorptionlorentz Lorentz function for modeling absorption (equivalent width).
absorptionvoigt Voigt function for modeling absorption (equivalent width).
accretiondisk A model of emission due to an accretion disk.
atten Model the attenuation by the Inter-Stellar Medium (ISM).
bbody A one-dimensional Blackbody model.
bbodyfreq A one-dimensional Blackbody model (frequency).
beta1d One-dimensional beta model function.
beta2d Two-dimensional beta model function.
blackbody Emission from a black body.
box1d One-dimensional box function.
box2d Two-dimensional box function.
bpl1d One-dimensional broken power-law function.
bremsstrahlung Bremsstrahlung emission.
brokenpowerlaw Broken power-law model.
ccm Galactic extinction: the Cardelli, Clayton, and Mathis model.
const1d A constant model for one-dimensional data.
const2d A constant model for two-dimensional data.
cos One-dimensional cosine function.
delta1d One-dimensional delta function.
delta2d Two-dimensional delta function.
dered A de-reddening model.
devaucouleurs2d Two-dimensional de Vaucouleurs model.
disk2d Two-dimensional uniform disk model.
edge Photoabsorption edge model.
emissiongaussian Gaussian function for modeling emission.
emissionlorentz Lorentz function for modeling emission.
emissionvoigt Voigt function for modeling emission.
erf One-dimensional error function.
erfc One-dimensional complementary error function.
exp One-dimensional exponential function.
exp10 One-dimensional exponential function, base 10.
fm UV extinction curve: Fitzpatrick and Massa 1988.
gauss1d One-dimensional gaussian function.
gauss2d Two-dimensional gaussian function.
hubblereynolds Two-dimensional Hubble-Reynolds model.
jdpileup A CCD pileup model for the ACIS detectors on Chandra.
linebroad A one-dimensional line-broadening profile.
lmc LMC extinction: the Howarth model.
log One-dimensional natural logarithm function.
log10 One-dimensional logarithm function, base 10.
logabsorption Gaussian function for modeling absorption (log of fwhm).
logemission Gaussian function for modeling emission (log of fwhm).
logparabola One-dimensional log-parabolic function.
lorentz1d One-dimensional normalized Lorentz model function.
lorentz2d Two-dimensional un-normalised Lorentz function.
normbeta1d One-dimensional normalized beta model function.
normgauss1d One-dimensional normalised gaussian function.
normgauss2d Two-dimensional normalised gaussian function.
opticalgaussian Gaussian function for modeling absorption (optical depth).
poisson One-dimensional Poisson function.
polynom1d One-dimensional polynomial function of order 8.
polynom2d Two-dimensional polynomial function.
polynomial Polynomial model of order 5.
powerlaw Power-law model.
powlaw1d One-dimensional power-law function.
recombination Optically-thin recombination continuum model.
scale1d A constant model for one-dimensional data.
scale2d A constant model for two-dimensional data.
schechter One-dimensional Schecter model function.
seaton Galactic extinction: the Seaton model from Synphot.
sersic2d Two-dimensional Sersic model.
shell2d A homogenous spherical 3D shell projected onto 2D.
sigmagauss2d Two-dimensional gaussian function (varying sigma).
sin One-dimensional sine function.
sm Galactic extinction: the Savage & Mathis model.
smc SMC extinction: the Prevot et al. 1984 model.
sqrt One-dimensional square root function.
stephi1d One-dimensional step function.
steplo1d One-dimensional step function.
tan One-dimensional tan function.
xgal Extragalactic extinction: Calzetti, Kinney and Storchi-Bergmann

Are models evaluated at a point or across a bin?

The integration of models in Sherpa is controlled by an integration flag in each model structure. Refer to "ahelp integrate" for information on integrating model components.


Bugs

See the bugs pages on the Sherpa website for an up-to-date listing of known bugs.

See Also

models
list_model_components, list_models, load_xscflux, load_xsclumin, load_xscpflux, load_xsgsmooth, load_xsireflect, load_xskdblur, load_xskdblur2, load_xskerrconv, load_xslsmooth, load_xspartcov, load_xsrdblur, load_xsreflect, load_xsrfxconv, load_xsrgsxsrc, load_xssimpl, load_xsvashift, load_xsvmshift, load_xsxilconv, load_xszashift, load_xszmshift, tablemodel, xs, xsconvolve