SSC Meeting Minutes 15 October 2001 Bolte, Miller, Nelson UCSC ) Taylor, Mclean, Quirrenbach, Chaffee, Beckers UCLA Steidel Keck Headquarters Mumma via phone Not in attendence, Ellis, Djorgovski, Luppino (note three-way video connection) also present, David Cowley, Steve Vogt, David Koo, Matt Radavan (UCSC) Greg Wirth (Keck) James Larkin, Jim Beletic, Hilton Lewis, Dave Sprayberry (UCLA) -Announcements .Keck Science meeting help October 13 at CIT, attendence ~80 .DEIMOS preship set for 13/14 November ship 11 Jan 1st light 28 April -HIRES upgrade (Steve Vogt) .updated budget presented .will be Leach II controller .dewar window/field flattener is designed, fused silica blank is in hand to be figured by Dave Hilyard in the Lick Optical shop .very likely to use CCDs from the three MIT-LL MBE wafers CARA owns. The decision about AR coating is important. Single coat hafnium-dioxide is superb in the blue/UV fringes in the red. Possibly use chips with two different AR coatings, one for the blue side, one for the red. There are 6 CCDs per wafer. (1) investigate AR coating the wafers one at a time, evaluating the first, deciding on the second, evaluating the second, deciding on the third. May want to keep in mind that we will be wanting new CCDs in LRIS-R soon. (2) Excellent blue/UV response is a high priority. .there was some discussion of going to a closed-cycle cooler, general consensus was that this is not a good idea to pursue. .Joe Miller offered a fixed-price contract at the budget+contingency with a payback if it is delivered below the maxium total. We accept. - ADC (Koo, Radovan) .Team request funding for a Phase A design of a LRIS-only ADC. .Will start with a pan-chromatic, fused silica, 2-prism design. *.We need to dig out the scientific requirements. - OSIRIS mini-review . James Larkin gave a two-hour presentation addressing the questions brought up after the PDR in July: >detectors >end-to-end simulations for sensitivity analysis >project management >data pipeline reduction .Detectors, 2kx2k HgCdTe Hawaii 2 with 2.5micron cutoff is the device of choice. Dominating factor for noise is the dark-current. Rockwell will allow hand picking of detectors for a charge (~50k). Shooting for <0.05e-/sec/pixel. There may also soon be an option for MBE devices with AR coating. Better QE, again higher cost. .Sensitivity. An end-to-end simulator is completed. The question marks about cross-talk (OH in one spectrum ending up in an adjacent spectrum) were addressed (it is a small problem). The bottom line is that OSIRIS is more sensitive than NIRSPEC or NIRC2 by alot - in part because of detectors, in part because of lack of slit losses, in part because of high total throughput (13% including AO). .Project management and detailed WBS. Larkin argued that the distribution of management in the project and the success of NIRSPEC with the same PI/projector manager (Ian in that case) approach says they will be OK. The SSC has doubts but the project will go forward with its current structure. *.DRP. The SSC asked for a more complete data reduction pipeline. Krabbe has come on the team and will head up this part of the effort. There is an added cost, we need to have a full spec for the final product. .Note that SHARC has become an integral part of OSIRIS. Steidel requests that the SHARC expenses be report with the OSIRIS budget in the future. -CARA report