Matt Craig

I'd lean towards the ccdproc/nddata work since there is other work being in astropy to adopt the array API.

Technically, both are still maintainers but Michael has stepped back and Steve is stretched pretty thin.

@embray -- any chance you could expand expand the instructions at http://docs.astropy.org/en/latest/development/workflow/maintainer_workflow.html#using-milestones-and-labels to explain how labels should be used? Or if you want new maintainers to stay away from that...

I think @somilia is the only one that needs to be added -- it is the fact that the person who opened the PR isn't part of the org that...

Looks like @lmichel is the only other committer...

@astrofrog @cdeil -- what is the status of flux conservation in reproject? We're getting ready to add a convenience function in ccdproc for combining images by reprojecting and I want...

I think I understand...so if I have an image in ADUs or photon counts I need to divide by pixel area, reproject, then multiply by pixel to get back to...

I think the fix is to convert the data to `float32` on the python side before sending the data to glue and friends...

Actually, maybe that isn't it....I see this if I create an image mark without _any_ data. Setting the data later doesn't seem to generate a complaint.

On my list for sprinting next week 😀. This is mostly javascript and acts as a drop-in replacement for the `Image` mark in bqplot. I had started trying to work...