We have written a report on GRIM II exposure timing and non-linearity. The gist of our report is: (a) The exposure time is currently OPENTIME + 0.901 +/- 0.006 seconds and is about 0.2 seconds less than the requested time. It appears that the exposure timing changed sometime between October 1994 and April 1996, but we do not know when. (b) The corrections for non-linearity are well-determined and can be as large as 10%. We have written an IRAF task to perform the correction. (c) It is fairly easy to expose past the working range of about 28000 DN because of the reset-read-read mode in which the array operates. Uncorrectable saturation can occur at levels as low as 13000 DN. We present a graph of the maximum safe exposure as a function of exposure time. The report can be obtained from ftp://oldp.nmsu.edu/pub/alan/grim/lin.ps.Z. We welcome comments. Alan Watson (awatson@nmsu.edu) Nancy Chanover (nchanove@nmsu.edu) APO APO APO APO APO Apache Point Observatory 3.5m APO APO APO APO APO This is message 20 in the apo35-grim archive. You can find APO the archive on http://www.astro.princeton.edu/APO/apo35-grim/INDEX.html APO To join/leave the list, send mail to apo35-request@astro.princeton.edu APO To post a message, mail it to apo35-grim@astro.princeton.edu APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO