Greetings. I have posted two new images that I captured with my Obsession and Mallincam Universe At Zephyr Ridge Observatory. (You need to scroll to the bottom to see the latest images.)
NGC457, the so-called Owl Cluster in Cassiopeia, is a well-known target for visual observers and is an easy target for astrophotography. I integrated 383 exposures, each of 10 seconds duration, to achieve the final result. The data was acquired on November 15, 2014. I used Pixinsight for all processing.
The second image is a far more challenging venture. The primary object is NGC3718, a distorted spiral galaxy also known as Arp 214. Very likely the gravitational disruption of NGC3718 is due to the companion galaxy NGC3729 (seen at the bottom of my image), which is located a mere 150 thousand lights years from NGC3718. The two galaxies are about 52 million light years from Earth. To the right of NGC3718 is Hickson 56, a cluster of five interacting galaxies that are about 400 million light years from Earth.
My image is the result of integrating 1244 exposures, each of 10 seconds duration, taken over four nights in April, 2015. It took a great deal of effort to acquire and process this many exposures, and yet the result is not as revealing as I had hoped. I was unable to capture the faint, swirling extensions of the spiral arms in NGC3718 that is seen in other images, although a faint hint can be seen in my image in the direction of the Hickson group.
I think this result highlights the limitations of my setup. Since I have restricted my exposures to 10 seconds to minimize the consequences of poor tracking (for astrophotography) and field rotation, the result is subject to more camera read noise as well as noise from the sky background. Perhaps adding more data would improve the result, but a tracking system that allows for longer subs is clearly needed for such a challenging object. I processed the image three different times, trying different approaches in each, but was unable to improve upon the result posted here.