- sherpa.astro.ui.get_quality(id=None, bkg_id=None)
Return the quality flags for a PHA data set.
The function returns the quality value for each channel in the PHA data set.
qual – The quality value for each channel in the PHA data set. This array is not grouped or filtered - that is, there is one element for each channel in the PHA data set. Changes to the elements of this array will change the values in the dataset (is is a reference to the values used to define the quality, not a copy).
- Return type
sherpa.utils.err.ArgumentErr – If the data set does not contain a PHA data set.
Fit one or more data sets.
Return the grouping array for a PHA data set.
Return the independent axes of a data set.
Exclude channels marked as bad in a PHA data set.
Load the quality array from a file and add to a PHA data set.
Apply a set of quality flags to a PHA data set.
The meaning of the quality column is taken from 1, which says that 0 indicates a “good” channel, 1 and 2 are for channels that are identified as “bad” or “dubious” (respectively) by software, 5 indicates a “bad” channel set by the user, and values of 3 or 4 are not used.
“The OGIP Spectral File Format”, https://heasarc.gsfc.nasa.gov/docs/heasarc/ofwg/docs/spectra/ogip_92_007/ogip_92_007.html
Copy the quality array from the default data set to data set 2:
>>> qual1 = get_quality() >>> set_quality(2, qual1)
Return the quality array of the background component labelled 2 for the ‘histate’ data set:
>>> qual = get_quality('histate', bkg_id=2)
Change the quality setting for all channels below 30 in the default data set to 5 (considered bad by the user):
>>> chans, = get_indep() >>> qual = get_quality() >>> qual[chans < 30] = 5