APO 3.5-m Users Committee Phonecon, 11/28/05 Attending: Suzanne Hawley, Jill Knapp (for Michael Strauss), Remy Indebetouw (for UVa), John Bally, Rene Walterbos, Bruce Balick, Bruce Gillespie Absent: Don York, Jon Holtzman, Karl Glazebrook, Al Harper, Russet McMillan Minutes taken by Bruce Gillespie ********************************** User feedback, comments from Institutional representatives: Princeton (Jill Knapp, for Michael Strauss)--Jill reported she had heard of no feedback from users. Colorado (John Bally)--John said his users had one issue. It appears that DIS spectra may be out of focus. Rene added that there is still the issue of scattered light in the blue channel. ACTION: Suzanne and BruceG will discuss this in the upcoming weekly operations telecon. NMSU (Rene Walterbos)--Rene reiterated the need to address the DIS focus and scattered light issues. Johns Hopkins--no report given. Chicago--no report given. UWashington (Bruce Balick)--BruceB said he had heard no input from users. He said there is anticipation at UW of the forthcoming report from the Futures Committee. Suzanne added that there is engineering time next week that will address some of the ongoing engineering issues. Univ. of Virginia (Remy Indebetouw)--Remy said he hadn't heard any user feedback. ********************************** Board of Governors meeting: Rene stated that it was a good meeting; the requested budgets were approved, and Ed Turner was elected as the incoming Board Chairperson, the Executive Council of the SDSS-II Advisory Council was formed, and there was an interim report from the Futures Committee. He also said that he had finished compiling the publications/theses list for the 3.5-m, which shows there were more papers/theses in 2005 than in 2004. Suzanne added that she also thought it was a successful meeting, and in particular she was pleased that the Board approved the UVa buy-in and the share adjustments that enable CU to double its share. ********************************** Town Meeting summary: Suzanne announced that all the ARC institutions had been personally visited by herself and BruceG during the past year, as part of Suzanne's orientation during her first year as 3.5-m Director. This afforded an opportunity for the 3.5-m users to hold direct discussions with us on telescope, instrument, and operational topics. One of the common topics heard from users at several institutions is the need to improve site user information. Within the manpower limitations we have, user information has been given a higher priority. Suzanne feels these meetings were very productive, and she thanks the individuals who participated and/or hosted the visits. BruceG mentioned that we don't intend to do this much traveling in future years, but that we would try to find opportunities to return to the ARC institutions, perhaps at a rate of ~one per year. ********************************** Discussion of telescope/instruments report: BruceG summarized highlights from the report (see below). ************************* 3.5-m Telescope, Instruments, and CIF Projects Highlights, 10/14 through 11/22/05 Bruce Gillespie 0) Overview This period saw effort expended in preparations for the annual Board of Governors meeting and planning for 2006, plus various work related to some instrument and telescope problems. The unusually good weather for this time of year was largely well used for observing. 1) Telescope In mid-October, it was discovered that the center-post support of the tertiary mirror had come unbonded from the glass. The telescope was shut down and the mirror and supports were removed. There was minor damage to the glass on the back surfaces of the mirror, which we were fortuitously able to have repaired quickly at the optical shop at the White Sands Missile Range. The support was rebonded to the mirror and telescope was brought back in service with only six nights of observing time lost. The cause of the glue failure is unknown, but is suspected to be due to age and/or possibly a defective bonding joint which failed. In November, the telescope developed small tracking oscillations that were determined to be related to the azimuth direct-drive boxes. These were removed and serviced, with the telescope returned to an operational state, with minimal down time. Also, the NA2 rotator bearing and mounts were serviced during engineering time, and the rotator performance has been improved, although one rotator motor overcurrent event was recently observed. At the moment, the telescope is performing nominally. 2) Instruments o NIC-FPS: The vacuum-leak problem in the NIC-FPS dewar persists. CU engineers came to APO, and a new LN2 fill gasket was installed which seemed, at first, to solve the problem. But in subsequent use the vacuum-leak problem returned and the instrument was taken out of service. Further testing and repairs are currently in progress. o CorMASS: The "flip mirror" became intermittent and UVa staff came to APO to effect repairs. The instrument appears to be working normally at this time. 3) Engineering and CIF projects Some progress was made on assembling the new drive boxes, and on analysis and design of the new top-end components. Work was slowed somewhat by manpower limitations due to telescope problems and vacation leave. 4) Miscellaneous 4th Observing Specialist position recruitment continued; three candidates were interviewed. A hiring decision is expected shortly. ********************************** Triplespec review: Suzanne announced that we are about to hold a final design review for the UVa NIR spectrograph called Triplespec. The review team is headed by Alan Uomoto, and the review will be held at the Sunspot Visitor Center 6-7 December. In addition to APO staff, Steve Smee (JHU), Tom O'Brien (OSU), Al Harper (UC), Fred Hearty and Stephane Beland (CU), and Craig Loomis (PU) plan to participate. Remy reported that the review preparations are going well; everything is just about ready to go. ********************************** CorMASS, APOLLO, GRB updates: BruceG said that CorMASS is at APO in working condition, and we expect it to remain available for users (in "attended-service mode") for the foreseeable future. APOLLO had success in getting return lunar photons during their November run. Suzanne reported that the GRB alert program has not been implemented recently, largely due to NIC-FPS being down because of its vacuum problems. ********************************** 3.5-m data access, security: When TUI was launched earlier this year, various firewall problems caused numerous problems with data transfers between APO and the ARC institutions. A website transfer system was implemented to get around this problem, but this solution inadvertently created a situation where all the 3.5-m data could be accessed publicly. The web-based data-transfer system has since been reverted to a more secure mechanism, while the ftp protocol remains the most commonly used by users anyway. But this incident has raised some issues, such as: Do we care if our data is available public (probably yes)? Do we care if ARC users have access to data not from their own observations? Should we allow public access to our data (or a catalog) after some TBD proprietary period? After some discussion, it was decided that the Users Committee members should poll their respective users: ACTION: Users Committee members should poll their users to ask if the the present data distribution/security systems at APO are adequate, and if not, why. ACTION: Users Committee members should poll their users to ask if we should permanently archive all 3.5-m data, and possibly make it available to the public, and if so, why. ********************************** Open actions from previous meetings: ACTION: Once we collect the the names of the designated institutional systems administrators, BruceG will have them listed on the APO web pages for reference. STATUS: will be completed in December. ACTION: BruceG will write a paragraph about the importance of having back-up programs, to be added to the e-mail automated message we send observers prior to their runs. STATUS: will be completed in December. ********************************** Next Users Committee phonecon will be on Monday, 23 January, at 8:30 AM Pacific Time. Agenda and other materials will be sent to the committee members during the preceding week. APO APO APO APO APO Apache Point Observatory 3.5m APO APO APO APO APO This is message 938 in the apo35-general archive. You can find APO the archive on http://www.astro.princeton.edu/APO/apo35-general/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-general@astro.princeton.edu APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO APO