Comments (2)
I think it might happen because a fit actually failed this time (or maybe it did work), but an existing file with the exact same name is already present and is read in. I'm going to try and improve the logic in the fit running function to make sure it doesn't happen.
The spectral fitting storage is garbage in XGA currently though
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I think the problem is specifically happening when the second time it is being run (with fewer spectra than some successful earlier analysis), the spectral fit finds that no spectra are suitable for fitting. This prints:
"No acceptable spectra are left after the cleaning step"
Which is a message I added, but it isn't picked up as an error by the parsing - I'll change the error message so that it should be caught.
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Related Issues (20)
- Add an inverted power law model to enable simple flipping of scaling relations
- An XMM + eROSITA sample is assigning an XMM image to the wrong source (it doesn't have that ObsID) HOT 8
- Getting an argument list too long error from spectrum generation HOT 4
- Overdensity radius measurement system (a la hydrostatic mass profile method) for the gas mass profiles HOT 3
- Tx and Lx get methods should except any product not available errors
- Timeout warnings for XSPEC fits should be lumped together and given at the end
- BaseSample nHs calls np.Quantity for some reason
- Why have a separate _shape attribute in Image - just dynamically get it from _data??
- Used Euclidean rather than Haversine distance in the offset calculation in 'offset' method of BaseSource
- Implement the LoVoCCS centroid measurements actually in XGA (rather than in a notebook) when I'm happy they are as automated as possible
- Review ClusterSample name checking and why I'm doing it
- Not sure radii-based retrieval of combined projected met profiles works
- Unintended behaviour - profiles have save_view() but aggregate profiles still has save_path argument in view
- Duplicate events in different eRASS Obs_IDS HOT 8
- Change the name of the LT pipeline in XGA
- get_interloper_mask(telescope='erosita') returns unhelpful error
- Retrieving existing SB/dens profiles is very hit or miss
- Some eRASS observations might not have data from all TMs HOT 1
- eRASS census being built with 0.0 DEC_PNT column but proper value RA_PNT column HOT 1
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