Comments (1)
Any new functions I do do this, and will slowly convert existing functions as I find them
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Related Issues (20)
- MPE-IKE border regions in eRASS are going to cause problems HOT 4
- eROSITA default image boundaries decision
- Stacked spectra don't necessarily seem to be loaded in on redeclaration for eROSITA
- XGA-LTR has a logical flaw
- EventList should support the reading in of event tables
- EventList should be able to generate XGA Image instances
- Allow the user to control the timestep for eROSITA spectrum generation - and include it as a retrieval criteria (i.e. along with min_counts)
- Make sure no XGA-spawned command line process copies any core.xxxxxx files out of the temporary directories
- Review the catch-all size for eROSITA CalPV fields that aren't eFEDS
- Review how best to return a single peak coordinate
- Need to do some proper profiling to see what improvements can be made to source/sample declaration efficiency
- None has no attribute usable can still pop up with AnnularSpectra definition HOT 1
- LoLSS analysis threw up an odd problem where the spectral read in gets the name of the spectrum for a coordinate
- Let GalaxyCluster instances store/use an overdensity radius error
- Check I didn't make XGA get stuck in ObsID specific directories in the existing products read method
- Could save the debug images as pngs rather than fits
- Brightness profiles still have stupid radius values and errors
- Maybe add a nice for model instances to show their fitted parameters
- 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 6
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