
Heart Nebula IC 1805 with the DWARF 3
A 3 hour 52 minute DWARF 3 session on the Heart Nebula (IC 1805) in Cassiopeia using the Duo-Band filter under Bortle 6 skies. Documents the challenge of imaging a large emission…
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Settings & Calibration · Processing · Imaging Sessions · Draco

A 3 hour 52 minute DWARF 3 session on the Heart Nebula (IC 1805) in Cassiopeia using the Duo-Band filter under Bortle 6 skies. Documents the challenge of imaging a large emission…

A 2 hour 54 minute DWARF 3 session on the Horsehead Nebula (B33) and Flame Nebula (NGC 2024) using the Duo-Band filter under Bortle 6 skies. Documents the challenge of imaging a…

DwarfLab recently added a dedicated Star Trail Mode to the Dwarf 3 app. This is my first test of it. 720 frames at 30 seconds each, six hours total, stacked in real…

A single-session DWARF 3 imaging project on M101, the Pinwheel Galaxy in Ursa Major. 6 hours and 18 minutes of total integration at 60-second sub-exposures, gain 50, Astro filter, Bortle 6. Documents…

A three-session DWARF 3 imaging project on M106, a Seyfert galaxy in Canes Venatici. 15 hours and 31 minutes of total integration, four companion galaxies in the field including NGC 4226 at…

A 30-minute M45 Pleiades capture on the DWARF 3 reveals why running denoise, star correction, and Auto in Stellar Studio then finishing in Snapseed with Adjust, Dehaze, Curves, and White Balance produces…

A 15-hour DWARF 3 imaging project on M81 and M82 comparing short versus 60-second sub-exposures under Bortle 6 skies, with background galaxy UGC 5210 detected at magnitude 14.88.

The Rosette Nebula from Monaco with the DWARF 3 in EQ mode using the Duo-Band filter. 210 captured frames became 141 stacked frames for 2h 21m of integration from one of the…

A documented DWARF 3 solar imaging session from December 3rd, 2025. Covers what white-light solar imaging can and cannot show, how sunspot size was measured using DraftSight, and what the observation can…

To capture 60-second exposures with the DWARF 3, you must use Guided EQ Mode. By aligning the telescope with the Earth’s celestial pole, you eliminate field rotation and quadruple your light collection…