Caliban is an irregular outer satellite of Uranus discovered with the Hale 5m at Palomar in 1997 and is estimated to be 72km in diameter.  At a MPC-ephemeris V magnitude of 22.2 it is likely the faintest I can manage in my program to image satellites in the outer solar system. Even with three hours exposure, unfiltered for maximum sensitivity, the signal to noise ratio is barely 3. The image above has used truncated histogram equalization to maximize the contrast.  Stacking was made markedly easier because the satellite is near a stationary point as observed from the earth, moving less than two arcseconds during the 3-hour exposure.

The only reasons why I am certain of the identification are that it lies exactly at the predicted position and there is no other object of comparable brightness at that position in any images taken to that limiting magnitude which I have been able to find.

Caliban was predicted to be at 02:01:03.0 +11:44:22 throughout the observation.  The brightest star in the image, to Caliban's upper left, is Gaia-DR2 2574537812519595520, with g-magnitude of 17.04, at 02:0107.3 +11:45:49.  The 2 stars below Caliban are magnitude 19.78 and 19.18 in Gaia-DR2.