astrofrog / astrofrog/sedfitter
Subsequent fitting after filter_output()?
- Dominant language
- Python
- Stars
- 21
- Forks
- 23
- PR merge metrics
- No merged PRs in 30d
Description
Hi Tom,
Looking for some features from the old fortran version that I found useful, perhaps you've implemented them somewhere already but I've missed it in the documentation...
Do you have a utility to produce new files in the fitter data format from the binary output.* files? Like the old fits2data when the output files were fits tables?
Also would be helpful if filter_output printed the number of well-fit and poorly-fit sources to the terminal, I've always found this to be a useful sanity check when fitting large batches of sources.
Cheers,
Matt
Contributor guide
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Research direction
Start by inspecting the existing filter_output entry point and the documentation for binary output.* files and the fitter data format. Check whether an existing utility corresponds to the old fits2data tool, then determine the expected output and terminal reporting behavior. Done means the requested conversion path and well-fit/poorly-fit source counts are clearly supported and documented.
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Assessment
- Tech stack
- python
- Domain
- data
- Issue type
- Feature
- Difficulty
- 4/5
- Estimated time
- 3-5 days
- Activity status
- Stale
- Clarity
- Needs clarification
- Newbie friendliness
- 25/100