Fellow users of DIS, As you all well know, the read noise on the red arm of DIS has been rather high (and variable) lately. The RN had reached 40 electrons, which was mostly due to the fact that the bias histograms are doubled peaked (actually they are sometimes triply peaked). On 22 August 1998 (UT) Jon Brinkman and Jim Gunn (others?) took a look at DIS to see if they could resolve the problem. The power supplies were swapped and other ones were tried as well. The end result is that the problem and the solution to it are still not clear, but DIS has been left in a state that is far better than it was found in. The reason for this note is to report new values for the RN and gain, since the gain on the red side has changed considerably as a result of a new power supply which operates at a different voltage. On the night of the changes, Tia and I found: Gain(electrons/ADU) RN(ADU) Blue 0.992 9.238 Red 1.497 6.788 Where the errors are certainly larger than the 3 decimal places that I give the numbers to. As of last night, the blue RN is stable at about 9.5 electrons, but the red RN is up to 14.3 electrons and is starting to show a double peak in the bias histogram. Jon Brinkman is looking into this continued change on the red side, but for now it is certainly better than it has been and the blue side is really quite nice. Gordon APO APO APO APO APO Apache Point Observatory 3.5m APO APO APO APO APO This is message 65 in the apo35-dis archive. You can find APO the archive on http://www.astro.princeton.edu/APO/apo35-dis/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-dis@astro.princeton.edu APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO