In this post, I will share the objects shot with the EQ6 R Pro + RC8 setup. Below is the list of equipment and software details used for all the images in this post. All these images are shot with a monochrome camera with LRGB and SHO (Sulphur, Hydrogen, and Oxygen) filters and combined during post process.
Equipment Details:
EQ6 R Pro Equatorial mount
GSO RC8 telescope at 1250mm focal length (with reducer)
ZWO ASI 2600MM Pro monochrome camera
ZWO OAG
ZWO ASI 174mm guide camera
ZWO 7x36mm filter wheel
Antlia LRGB V Pro filters
Antlia 3nm SHO filters
Pegasus Power Box Advance (for power distribution)
Software:
N.I.N.A for capturing
PixInsight for stacking and processing
Lightroom for final processing
ARP273 - The Cosmic Rose
ARP 273 is a pair of interacting galaxies 350 million light years away in the Andromeda constellation. The larger of the galaxies is named as UGC1810 and it's smaller companion UGC1813.
The outermost arm of the larger spiral appears to have been pulled into a wide ring around the galaxy — a characteristic astronomers often see in galaxy pairs where one galaxy has passed through the other. The ring around this galaxy is off-center, though. This suggests the smaller galaxy plunged through the larger one
It is thought that the smaller galaxy has gone through the larger galaxy. The encounter seems to have also tipped the large galaxy's inner arms relative to the rest of the galaxy, while the smaller galaxy has become somewhat stretched out, with two sprawling tails on either end.
Exposure Details: 5 hours 35 minutes
L - 37 * 300 seconds
R - 10 * 300 seconds
G - 10 * 300 seconds
B - 10 * 300 seconds
Some interesting facts on this image: - I processed this image on the 13th of February and sent this to my wife for Valentine's day

- This is the farthest object I have shot intentionally and with details (earlier, I had unintentionally captured a small galaxy in the Hercules Globular cluster, which is about 500 million light-years away). The light that I have shot today left these galaxies 350 million years before. These galaxies may have moved farther away from us and also between each other now.
- This image looks smudged and lacks details because of the distance and the size of the object. The below picture shows the full frame in the L channel. Note how small an area these galaxies occupy.

My wish is to shoot this target in more detail with a longer focal length. I have ordered a 9.25" EdgeHD telescope with a focal length of 2350mm. I will revisit this target next year with this focal length.
ARP316 / HCG 44
Scanning the skies for galaxies, Canadian astronomer Paul Hickson and colleagues identified some 100 compact groups of galaxies, now appropriately called Hickson Compact Groups. The four prominent galaxies seen in this image are one such group, Hickson 44, about 100 million light-years distant toward the constellation Leo.
The two spiral galaxies in the center of the image are edge-on NGC 3190 with its distinctive, warped dust lanes, and S-shaped NGC 3187. Along with the bright elliptical, NGC 3193 at the bottom right, they are also known as Arp 316. The spiral in the upper left corner is NGC 3185, the 4th member of the Hickson group. Like other galaxies in Hickson groups, these show signs of distortion and enhanced star formation, evidence of a gravitational tug of war that will eventually result in galaxy mergers on a cosmic timescale. The merger process is now understood to be a normal part of the evolution of galaxies, including our own Milky Way. For scale, NGC 3190 is about 75,000 light-years across at the estimated distance of Hickson 44.
Two dwarf spiral galaxies named PGC 86788 (left center) and PGC 2806871 (top right) are also part of the group but are not included in the Hickson catalog
Exposure Details: 9 hours 21 minutes
L - 216 minutes (72 * 180 seconds)
R - 120 minutes (24 * 300 seconds)
G - 120 minutes (24 * 300 seconds)
B - 105 minutes (21 * 300 seconds)
This is my most favorite image from this trip.
NGC 2903 - A Barred Spiral Galaxy
NGC 2903 is an isolated barred spiral galaxy in the equatorial constellation of Leo. It was discovered by German-born astronomer William Herschel, who cataloged it on November 16, 1784. This galaxy is located about 30 million light-years away from the Milky Way and is a member of the Virgo Supercluster.
Exposure Details: 4 hours 21 minutes
L - 1 hour 51 minutes (37 * 180 seconds)
R - 50 minutes (10 * 300 seconds)
G - 50 minutes (10 * 300 seconds)
B - 50 minutes (10 * 300 seconds)
Abell 36 - Planetary Nebula
This gaseous shroud of a dying sunlike star, planetary nebula Abell 36 lies a mere 800 light-years away in the constellation of Virgo. At that distance it spans over 1.5 light-years. Shrugging off its outer layers, the nebula's central star is contracting and becoming hotter, evolving towards a final white dwarf phase. In fact, in Abell 36, the central star is estimated to have a surface temperature of over 73,000 K, compared to the Sun's present 6,000 K temperature. As a result, the intensely hot star is much brighter in ultraviolet light, compared to its visual appearance here. The invisible ultraviolet light ionizes hydrogen and oxygen atoms in the nebula and ultimately powers the beautiful visible light glow.
Exposure Details: 10 hours 55 minutes
Ha - 3 hours 40 minutes (44 * 300 seconds)
Sii - 3 hours 35 minutes (43 * 300 seconds)
Oiii - 3 hours 40 minutes (44 * 300 seconds)
Though I collected close to 11 hours of data (the longest for any target during this event), this image still lacks details and has lots of noise. Not a satisfactory result. Planetary nebulae are usually very dim and need lots of data to bring out the details and contrast.