The attached excerpt of a message from Lew Hobbs (UC) to me summarizes the current (late July '95) status of the Eschelle. Ed Turner ----------------------------------------------------------------------- 2) I promised to keep you apprised of the status of the echelle spectrograph. I just obtained today's update, and the punch line is that it's extremely unlikely that the instrument will be available to users before October 1. With virtually no risk (unfortunately), you can therefore begin to consider advising the five TAC chairs to dispose of the echelle time scheduled in September for their respective observers, in whatever ways we and you see fit. 3) In brief summary, the echelle problem continues to be what it has been for a number of months now: "poor" vacuum/cooling performance in the camera section. A layer of frost continues to form on the (vacant) CCD holder when the camera is cooled to the CCD operating temperature. The root cause is said to be the large ratio of the warm surface area of the camera housing to the cold surface area of the chip. There apparently is only one other camera known of similar design which has been made to work, after strenuous effort. I'm sure that none of us -- including the external expert who attended the critical design review years ago -- realized that we were sailing into previously uncharted waters. (No pun intended.) APO APO APO APO APO Apache Point Observatory 3.5m APO APO APO APO APO This is message 1 in the apo35-echelle archive. You can find APO the archive in /u/strauss/apo/mailer/apo35-echelle on astro.princeton.edu APO To join/leave the list, send mail to apo35-request@astro.princeton.edu APO To post a message, mail it to apo35-echelle@astro.princeton.edu APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO