200/250mm - 8" (7/28/19): at 107x; extremely faint, very small, required averted vision but I was able to often glimpse a ghostly, nebulous patch at the same position. It was slightly easier at 174x and showed a more definitive oval patch. Used 8" off-axis mask.

400/500mm - 17.5" (8/5/94): UGC 11672 was accidentally picked up while drifting 3.0 minutes east and 6' S of distant globular cluster NGC 7006. Faint, fairly small, elongated 5:2 ~E-W, 1.0'x0.4'. Contains a brighter core which at moments appeared double. This is an interacting galaxy with double nuclei separated by 15".

600/800mm - 24" (7/2/19): at 375x; overall this advanced merger appeared fairly faint, elongated, irregular, brighter on the eastern side. It often resolved into two cores (separated by 16") with the fainter core on the west side. Situated in a rich Milky Way star field 6' NNE of a mag 10 star, 25' ENE of mag 6.9 HD 200393 and 44' ESE of globular cluster NGC 7006.

24" (7/29/16): at 260x; overall this merged VV pair appeared fairly faint, moderately large, elongated ~2:1 E-W. The smaller and fainter western component bulges out slightly from the elongated eastern glow.

24" (7/21/12): this disrupted interacting system was easily resolved at 375x. The slightly brighter eastern component (VV 102a) appeared fairly faint, fairly small, ~30" diameter, but an irregular shape. The surface brightness is also irregular with a mottled, patchy appearance. The western component (VV 102b = LEDA 200369) is in contact at the edge of the halo and appeared faint to fairly faint, very small, round, 18" diameter. The two cores are just 16" apart.