Large Magellanic Cloud

Telescope Live is still building this dataset and I was able to add another two hours of observation data. That changed the processing results and the final image considerably - for the better. The dataset is still got a ways to go to get to the 15-20 minimum frame count per filter necessary to enable all the tool functionality in PixInsight. However, just this one additional set of data made a big difference.

I was now able to get a useable starless frame set to go with the Stars frame set. That allowed me to be work in greater detail/more agressively on the Starless data since the Stars were no longer being impacted. I feel it still needs some Oiii/Sii data to full represent the Tarantula Nebual and Cats Paw Nebula components of the LMC. I don't know if Telescope Live has any plans to get additonal narroband data from this OTA on this target, but it would be great if they did. IMO.

Wikipedia:
The Large Magellanic Cloud (LMC), or Nubecula Major, is a satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs (≈160,000 light-years), the LMC is the second- or third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal (~16 kpc) and the possible dwarf irregular galaxy known as the Canis Major Overdensity.

Based on the D25 isophote at the B-band (445 nm wavelength of light), the Large Magellanic Cloud is approximately 9.86 kiloparsecs (32,200 light-years) across. It is roughly a hundredth as massive as the Milky Way and is the fourth-largest galaxy in the Local Group, after the Andromeda Galaxy (M31), the Milky Way and the Triangulum Galaxy (M33).

The LMC is classified as a Magellanic spiral It contains a stellar bar that is geometrically off center, suggesting that it was a barred dwarf spiral galaxy before its spiral arms were disrupted, likely by tidal interactions from the Small Magellanic Cloud (SMC) and the Milky Way's gravity.

With a declination of about −70°, the LMC is visible as a faint "cloud" from the southern hemisphere of the Earth and from as far north as 20° N. It straddles the constellations Dorado and Mensa and has an apparent length of about 10° to the naked eye, 20 times the Moon's diameter, from dark sites away from light pollution.

The Milky Way and the LMC are predicted to merge in approximately 2.4 billion years