
A widefield shot of the famous Double Cluster from Sept 17th 2014 at Cherry Springs State Park. The Double Cluster is in Perseus but is in close proximity to Cassiopeia.


A widefield shot of the famous Double Cluster from Sept 17th 2014 at Cherry Springs State Park. The Double Cluster is in Perseus but is in close proximity to Cassiopeia.

I purchased one of the first Apogee Ascent A694 Cameras (Sony ICX694 Chip) before the acquisition by Andor and had some random horizontal banding across the top of the frame that was not possible to calibrate out:

Andor issued an RMA and took care of the costs under warranty. They stated that they repaired the camera by replacing the whole electronics board.
I was hoping to not see the random horizontal bands again but upon firing up the camera and cooling down to -15C there were still there although they are now contained in a smaller region closer to the top of the frame. It still moves around so calibration is difficult if not impossible. When using a small number of frames it is hard to statistically reject the band. You can see below in M42, reproduced at 50% size, that a bright band stands out across the top of the bias and dark calibrated image even after calibration. This is especially obvious in narrowband images where the background pixel count isn’t much higher than the bias floor. The band is also visible across the bottom of the Horse Head shot (I flipped the image) although it doesn’t stand out quite as much.
For a low bias noise camera geared towards narrowband imaging that I plan to use for portable imaging (lower frame count) I don’t think that my options are too great:
I am also including 100% size images of the bias, master bias, dark, and master darks used to calibration the two trial images.


Here is what several bias frames look like animated to give you an idea how the horizontal banding moves around and therefore is not well calibrated:
This is certainly better than what it was before but I am still left with these bands appearing faintly in my images.
All images were captured with the CCD cooled to -15C. They were captured with MaximDL 5 and calibrated / processed in Pixinsight.
I began work on a tri-color Hubble Pallet image during the summer of 2014 but due to weather and other obligations did not capture much in the way of Oxygen [O III] and Sulfur [S II] emission data for the mosaic project so am leaving it as a monochrome image using only the Hydrogen Alpha emission line data.

