A brief description of the equipment can be found on the instruments page. Almost any of the images produced by the survey show faint nebulae that haven't been cataloged before (which does not mean they are unknown). An attempt to list these objects can be found on the Uncataloged objects page.
Milky Way from Perseus to Monoceros:
Orion-Eridanus Superbubble and dense molecular clouds
High galactic latitude nebulae around celestial north pole
Milky Way from Cygnus to Perseus:
Many prominent HII regions
Nebulae below the galactic plane
Milky Way from Aquila to Cygnus:
A region full of supernova remnants
Hundertwasser-Corner:
Nebulae that appear to be created using a ruler
Milky Way from Scutum to Aquila:
Star fields behind dark nebulae
SH2-27 (ζ Ophiuchi Nebula) behind molecular clouds
OIII arc in Gemini Milky from Perseus to Cassiopeia Milky Way in Cassiopeia and Cepheus HII region around California Nebula (NGC 1499) Milky Way in Cygnus Milky Way from Vulpecula to Aquila Milky Way from Scutum to Ophiuchus Orion region Milky Way from Taurus to Perseus M33 to SH2-126 Milky Way from Monoceros to Gemini
For optimal display, the monitor should be calibrated so that as many shades of the grayscale shown below are distinguishable. At least the 4% steps should be separated by every monitor. The 2% steps are visible on better monitors. To distinguish the 1% steps, a HDR monitor is required.