Output latex table of fitted emission lines and fluxes.
mdl2latex outputs a latex table containing data extracted from
Sherpa models. The table contains all emission lines fit
using a gaussian, lorentzian, or delta function model. The
wavelength, flux, and flux error is output, along with a list
of the data the line was fit to. Finally, if a line
identification has been given by the user (using the Sherpa
command name_of_model lineid "line identification"),
this is output as well. See also the GUIDE thread showing how to use GUIDE with grating data to
identify and describe emission lines.
mdl2latex is a GUIDE routine, which must be initialized
using the require("guide") command in Sherpa. GUIDE
uses the optional ATOMDB database, and
this command may fail if the ATOMDB is not available on your
system.
% after fitting some emission lines
sherpa> require("guide")
sherpa> g1 lineid "Fe XVII"
sherpa> g2 lineid "O VII R"
sherpa> g3 lineid "O VII I"
sherpa> g4 lineid "O VII F"
sherpa> mdl2latex
\begin{tabular}{lllllll}
ModelName & Line Model & Position & Flux & Flux Error & Fit Data &
Label \\
& & Angstrom & ph/cm$^2$/s & ph/cm$^2$/s & \\
g1 & normgauss1d & 15.01 & 301.31 & 10.83 & 3,4,9,10 & Fe XVII \\
g2 & normgauss1d & 21.6 & 54.31 & 3.13 & 3,4,9,10 & O VII R \\
g3 & normgauss1d & 21.8 & 10.38 & 1.01 & 3,4,9,10 & O VII I \\
g4 & normgauss1d & 22.1 & 48.91 & 5.13 & 3,4,9,10 & O VII F \\
\end{tabular}
Here we output all emission features fit using sherpa with
gaussians, lorenzians, or delta functions; in this case,
only normalized gaussians (normgauss1d) were used.
sherpa> require("guide")
sherpa> mdl2latex("table.tex")
% a file table.tex is written with the mdl data.
This outputs all emission features fit using sherpa with
gaussians, lorenzians, or delta functions to the file table.tex.
Parameter=filename (string not required filetype=input)
The filename to use when writing the latex table.
|
![[CIAO Logo]](../imgs/ciao_logo_navbar.gif){kind=logo}