- sherpa.astro.ui.save_source(id, filename=None, bkg_id=None, ascii=False, clobber=False)
Save the model values to a file.
The model is evaluated on the grid of the data set, but does not include any instrument response (such as a PSF or ARF and RMF).
ascii (bool, optional) – If
Falsethen the data is written as a FITS format binary table. The default is
False. The exact format of the output file depends on the I/O library in use (Crates or AstroPy).
clobber (bool, optional) – If
None, then this flag controls whether an existing file can be overwritten (
True) or if it raises an exception (
False, the default setting).
The function does not follow the normal Python standards for parameter use, since it is designed for easy interactive use. When called with a single un-named argument, it is taken to be the
filenameparameter. If given two un-named arguments, then they are interpreted as the
filenameparameters, respectively. The remaining parameters are expected to be given as named arguments.
The output file contains the columns
SOURCEfor 1D data sets. The residuals array respects any filter or (for PHA files), grouping settings.
Write the model values for the default data set to the file “model.fits”:
Write the model from the data set ‘jet’ to the ASCII file “model.dat”:
>>> save_source('jet', "model.dat", ascii=True)
For 2D (image) data sets, the model is written out as an image:
>>> save_source('img', 'model.img')