Cygnus Wall
In 2025, ZWO finally implemented an equatorial mode for its versatile Seestar telescopes. This opened up a whole new range of imaging possibilities. In August and September 2025, we used a Seestar S50 in EQ mode to shoot the sources for this image of the Cygnus Wall in NGC 7000. The luminance channel of the image came from 2 hours of 60 second exposures with the built-in dual-band filter. The color was obtained with another hour of unfiltered 60 second exposures. We processed the data with Siril and combined the channels with Photoshop. [Released December 7, 2025]