-
Sphinx doesn't like the way I have `sherpa.astro.xspec` included in the ReadTheDocs documentation (two separate pages, one for "functions" and one for "models"). I should re-write so there's only one …
-
When looking at energy flux from complex objects \(i.e. magnetars\), the calculation is often depending on xspec fits and models used.
A model independent energy flux calculation could be implement…
-
Currently, the default for LevMar, NelderMead, etc. is set to epsilon for single precision float `'epsfcn': 1.1920928955078125e-07`. Why was it chosen this way?
I don't think anyone still uses mac…
-
I am trying to update https://sherpa.readthedocs.io/en/4.14.0/developer/index.html#install-from-source-in-conda to work for CIAO 4.14. In doing so I noticed that we do not have a consistent naming sch…
-
This is a long-term goal I'd like done, but don't have time for and want to get my thoughts down so it isn't forgotten. If anyone would like to work on this I'd be more-than-happy to provide pointers!…
-
Once you've set the quality array of a DataPHA dataset and called `ignore_bad`, what should happen when you remove the quality array:
This is with CIAO 4.14 but it's the same in the current main br…
-
This issue is to start a discussion thread about fitting non X-ray datasets that might be injective, or have gaps in them. The specific example I have in mind is fitting radio to gamma ray data for a …
phajy updated
11 months ago
-
* BXA version: 4.0.5
* UltraNest version: 3.3.3
* Python version: 3.8.12
* Xspec version: 12.12.1
* Operating System: macOS Monterey 12.6
### Description
When using the BXA-generated chain f…
-
I forgot to check that the sherpa.astro.utils.xspec code works with recent updates to the XSPEC code. It looks like `model_to_compiled` needs to change - for FORTRAN code - from the
void name_…
-
Using this issue to track and plan the next features. Any additional, comment in this issue and this top post will be edited to include them, link to sub-issues, and list relevant PRs for each item.
…