APO 3.5-m Users Committee Phonecon, 3/31/08 Attending: Suzanne Hawley, Bruce Gillespie, Scott Anderson, John Bally, Mark Klaene, Al Harper, Jon Holtzman, Jon Fulbright, Michael Strauss, John Wilson and Mike Skrutskie (both sitting in for Remy) Absent: Remy Indebetouw, Russet McMillan Minutes taken by Bruce Gillespie ********************************** User feedback, comments from institutional representatives: Princeton (Strauss) - Michael said the PU users were happy, and he had not heard of any problems or issues. UVa (Indebetouw) - John Wilson (sitting in for Remy) had nothing new to report on user feedback or issues. UW (Anderson) - Scott had nothing new to report on user feedback or issues. CU (Bally) - John mentioned that CU has two Ph.D. theses finishing this semester, based on observations taken at APO. JHU (Fulbright) - Jon had nothing new to report on user feedback or issues. NMSU (Holtzman) - Jon had nothing new to report on user feedback or issues. UChicago (Harper) - Al had nothing new to report on user feedback or issues. ********************************** Discussion of telescope/instruments report - Klaene: The report is given below. Mark highlighted that the usual spring winds are kicking up dust, but the dust counts are not often reaching telescope closure levels (yet) as seen in previous years. There has been little precipitation in the past couple of months, and the forest is extremely dry. The Forest Service has just issued Level II (out of four) fire restrictions. As precautions, the dead grass surrounding the site has been mowed, firelines have been cut, and the outside water sprinkler system has been set up. The most significant recent issue with the telescope was the discovery and repair of a stuck secondary actuator, which seems to have been caused by a large ambient temperature swing. All the instruments are in good shape, and TripleSpec was delivered and started its commissioning. CorMASS was decommissioned and is being stored in the lower level of the telescope. The tertiary support rebuild project held its critical design review, and its implementation appears to be on budget and schedule for completion during the summer shutdown. The NA2 instrument rotator upgrade (both mechanical and controller) was completed and is now in service. Detailed planning for the summer shutdown is underway. Congratulations are in order for the APO technical and observing staff who contributed to all of these efforts during the past months, and to the TripleSpec development team. ************************* 3.5-m Telescope, Instruments, and CIF Projects Highlights, 2/021/08 through 3/23/08 Mark Klaene & Bruce Gillespie 0) Overview Operations continued largely routinely. We are approaching the beginning of spring weather with the normal high winds and elevated dust levels, which will be monitored closely and may affect opening and closing conditions over the next few months. The fire danger level in the surrounding forest is now very high and expected to reach the extreme level in upcoming weeks. Planning and work is already being done to enhance the protection of the observatory and staff in the event of a nearby forest fire. The SDSS-III construction for the expansion of the Support Building has been completed. 1) Telescope Due to a stuck secondary axial actuator (thought to be caused by a significant ambient temperature swing), the telescope was out of collimation for a few days. The axial actuator problem was corrected quickly, however the transverse actuators while reporting good values, were also apparently mis-positioned. Due to weather conditions at the time and confusion with the slit viewer being used to check collimation (which has its own intrinsic aberrations) the problem took a few days to find and correct. 2) Instruments DIS, SPIcam, and the Echelle operated smoothly throughout the period. The new fanout board for NIC-FPS has been received at CU and we are waiting for them to schedule a date to warm the instrument, install the fanout board, and remove the etalon for testing back at CU. We have proposed to do this work during time in April when NIC-FPS is not scheduled for observing. With the arrival of TripleSpec, CorMASS has been decommissioned and is no longer available for observations. The visiting instruments (GFP and APOLLO) were all operational. TripleSpec arrived at the observatory after a productive series of lab tests and cool-downs. Initial on-sky commissioning started ahead of schedule because of the rotator upgrade work and ended with a successful three nights of commissioning. Minor modifications will be required to make the instrument easier to mount and dismount, and TUI integration still needs to be completed along with improvements to guiding. 3) CIF projects We are progressing on the implementation of Agile field rotation and its migration to the TR2 mirror cell port. Design drawings have gone to the shop, and parts have been ordered or received. The Critical Design Review for the Tertiary support/actuator upgrade was held on March 6 and 7th. The project cost estimates are within the planned budget, and the work is on schedule for a planned August installation. The project was given a green light to proceed with only minor recommendations. The new direct-drive rotator motor and axis controller were installed just prior to TripleSpec commissioning run. Preliminary tests indicate that all objectives of the rotator drive upgrade have been met. Further testing, analysis and cleanup of hardware and software will continue over the coming weeks. 4) Summer Shutdown Planning is underway for the upcoming engineering shutdowns. The initial take is looking like two 3-day shutdowns (in June and July), and a 2- to 3-week shutdown in mid-August. All the shutdowns will be centered around bright time. ********************************** TripleSpec commissioning - Skrutskie, Wilson, Hawley: Suzanne was pleased to report that the delivery, installation, integration, and initial commissioning of TripleSpec has gone exceedingly well. The main part that needs to be finished is the TUI interface software, after which we hope to release the instrument to our general user community. This is likely to happen by May so that the instrument can be available for proposals for scheduled use in Q3. We encourage prospective TripleSpec users to talk to Mike Skrutskie and John Wilson at UVa about using the instrument. A preliminary user manual will be posted, and data reduction tools will soon be available. Regarding instrument performance, Mike Skrutskie said that TripleSpec shows very low read or dark noise, and produces a decent S/N spectrum on a 15th magnitude target in a few minutes exposure. Sky noise is the limit, as expected. We intend to soon try some tests going deeper, to ~18th magnitude. Suzanne asked that User Committee members inform their users of the upcoming availability of TripleSpec, and to encourage them to propose test targets to Mike and John for possible engineering test observations (shared-risk, non-proprietary) during April and May. We also plan to announce that some of the TripleSpec commissioning data already taken will be made available to the ARC community so that people can learn more about the capabilities of the instrument. As far as we know, only APO and Palomar have mid-sized telescopes that can take single-exposure, full-wavelength coverage NIR spectra. Again, our congratulations and appreciation go out to the UVa instrument developers and the APO staff for their hard work in reaching this outstanding accomplishment. ********************************** NIC-FPS status - Bally: John said that the new, low-noise, fan-out board for NIC-FPS has been fabricated. The schedule and arrangements to install the board at the site are being worked out, hopefully in May. At the same time as the fan-out board is replaced, the faulty Fabry-Perot etalon will be removed and returned to CU for analysis and repair. ********************************** Instrument rotator upgrade - Klaene: The upgrade to the NA2 instrument rotator was discussed in detail above in the Telescope/Instrument report. So far, it appears to be working very well (with higher torque and better motion control than the old rotator system); we ask that if any of our users see quirks in its behavior during their observing runs to please notify the APO staff. Bruce said that although this was largely an APO effort (kudos to Nick McDonald and Fritz Stauffer), we should also acknowledge and thank UVa for their significant support for this upgrade, which was in part needed to accommodate Triplespec. ********************************** Tertiary mount CDR, and autofocus - Klaene: Although also already discussed above, Mark added that the rebuild of the tertiary mount will be fairly straightforward (compared to the past rebuild of the top end and secondary mounts). When implemented this summer, we should see improvements in stiffness, mirror-position stability, maintainability, and safety to the glass. On the autofocus project, substantial progress is expected in the coming months, which will be reported on in future meetings. ********************************** Curation of NIC-FPS raw data - Hawley: Suzanne reminded the committee to inform their users that we are about to implement the policy of deleting all raw NIC-FPS data older than 90 days. This was discussed in detail at last month's meeting, and in early April we will purge all NIC-FPS raw data (but not the processed images) stored at APO that were taken before January '08. A separate announcement to this effect will be posted to apo35-general. ********************************** ACTION ITEMS: [open from previous months]: ACTION: John Bally will write a section with figures on Fowler sampling for inclusion in the NIC-FPS user documentation. STATUS: John will check to see if the Fowler sampling documentation has been posted and is adequate. [new actions from this month]: none ********************************** Next meeting: The next Users Committee phonecon will be on Monday, 28 April, at 8:30 AM Pacific Time. The 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 1097 in the apo35-general archive. 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