I thought I understood cc until I recently imaged my first star cluster (Hercules). I have learned the value of dither and drizzle to achieve a remarkable improvement in image quality with my otherwise undersampled OSC data on nebulae and galaxies. I had also been using cc by default to remove ~7sigma hot pixels.
However, my first integration attempt on the Hercules cluster resulted in horrible donut like bright stars all through the cluster. After some Googling, I simply dropped the CC step in WBPP and the drizzled stars became fine. The original “donut” stars were bright, but not saturated and I didn’t see the problem on brighter stars outside the cluster.
As this came up in as Google search, it seems to be a known effect, but I don’t understand what was happening and I’d really appreciate it if one of the PI experts on this forum could help explain.
Many thanks - Paul
Comments
I am rewatching the entire WBPP lessons again as I begin to appreciate the importance of really understanding this step in the process.
I’m now trying to get my head around the weighting process and whether/when adding a lower quality subframe improves or degrades the final result (ie: how do I decide quantitatively when to reject a sub/ frame).
-Paul