XGA
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DavidT3
X-ray: Generate and Analyse is a module designed to make the analysis of XMM observations simple and efficient. It provides an interface with SAS for the creation of XMM data products, as well as a wa...
It says 'default should be able to match a source on the edge of an observation to the centre of the observation.', but the default is 30 arcmin which is...
I don't know how this should be integrated into source declaration, or if it should, but allow for matching within some sort of match radius rather than making sure the...
This will be great, largely because of the need for XSPEC and SAS to be installed. That means I will be able to use CI tests easily in theory, and...
I'm not sure how valid some of the results I'm getting are with my hierarchical peak finder. Certainly it deals with point source remnants extremely well, but I have to...
The requirements of eRASS and other eROSITA data (the cal pv stuff) can be different enough that two different telescope names are justified. Sort of began this process in one...
By this I mean having a box in another part of the image away from the source, rather than an annulus around the source. For brighter point sources with big...
Primary configuration file - let a config file point to another centralised config file and use that
I.e. in the configuration file someone has in their local directory, the top section of the file could contain a 'PRIMARY_CONF' entry or some such, that could be populated with...
Currently we require there be an existing image (e.g. not one that XGA made) to convert regions to SkyRegions and check if the UDC is contained within any of them....
Don't yet know why, but they are simply not the same as Paul's uses of LIRA (checked on the same dataset) or compared to other measurements of scatter. May not...