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Attending: Nancy Chanover (NMSU), Chip Kobulnicky (UWy), Misty Bentz (GSU), Mukremin Kilic (OU), Russet McMillan (APO), Ben Williams (UW), Jamey Eriksen (APO), Eric Nielsen (NMSU), Aleksandr Mosenkov (BYU), Joanne Hughes (Seattle U), Anne Verbiscer (UVa), Derek Buzasi (FGCU), Kevin Schlaufman (JHU)
The detailed site report is included below, followed by additional information discussed during today's meeting.
3.5-m Telescope and Instruments Highlights, 8/01/2023 – 9/04/2023
1) Overview
It has been a very busy and exciting month at APO! Shutdown started in late July and culminated with the return to sky on 8/23. The mirror was successfully recoated at Lowell Discovery Telescope outside of Flagstaff. The team of Bill Ketzeback, Amanda Townsend, Riley DeColibus and Jamey Eriksen escorted the mirror to LDT, worked with the LDT team who cleaned, stripped and recoated the mirror in the LDT chamber, and then escorted the mirror back to APO.
In late August a visiting team from UVa for DSSI arrived at APO. In September we will host a visiting group from the Pacific Northwest, along with a group associated with the SDSS project for a software coding workshop.
2) Operations
3.5m Telescope:
The telescope returned to operations post-shutdown. The M3 rotation failure has been narrowed down to a failed high resolution encoder. A replacement has been ordered, a new mount is being fabricated and we anticipate being able to test the replacement encoder in 2 weeks. A plan is also being developed for an upgrade path for the M3 rotation system because of the obsolete parts in the system (the motors and motor encoders, which we have not been able to find spares for).
The telescope balance has been marginal after the removal of the LANL instrument. There is an occasional motion error during slews. So far no reports have been received about motion errors while tracking. Further refinements of telescope balance are ongoing.
Instruments:
- KOSMOS was warmed up during shutdown for a vacuum cycle with a getter recharge; the instrument is now cooled and operational.
- servicing of the ARCTIC diffuser rotator had to be postponed; it will be rescheduled for a later date.
- The Agile TEC controls failed. Princeton Instruments will no longer support the camera or controller hardware. Finding and ordering surplus equipment in an attempt to repair it has so far been unsuccessful.
- The ARCES inter-order light ratios (measure of scattered light in the instrument) are still good but are declining again in the warmer weather.
- The scattered light in the DIS red camera improved dramatically recently (attributed to a detector partial warm up) and the camera is considered to be very good. However, the blue camera is still considered sub-par.
0.5m Telescope: The filter wheel has failed. Attempts to repair it have so far been unsuccessful. A replacement filter wheel is being researched.
Very busy/exciting/stressful 2 months! Mirror successfully recoated at Lowell Discovery Channel Telescope. Will distribute data re: coating performance once reduced. DSSI team on site, SU collaborators here. SDSS coding workshop here. Telescope back in operations. M3 failure; replacement encoder being tested, working on coupler and mounting, hope to try in telescope tomorrow. Once functional will work on upgrade path to bring that system to newer tech. Hi res encoder easier than motor controller. Bill working on balance issue; still fine-tuning it. KOSMOS working. ARCTIC diffuser rotation ARCES IOL good but may decline DIS: red good, blue bad ARCSAT: filter wheel has failed Jack testing out PlanetCam idea on 0.5m - high speed imaging system
mirror perfomance in lab data being reduced and on sky data - photom conditions but very bad seeing - hard to compare
cyber attack we reevaluated our security - biggest hole is mail server at APO second thing: backups - everything backed up pn site to VM , now instituted off-site cloud back up for all critical systems now inventorying hardware if have replacements, install VM look at critical systems in observing control rooms most ransom ware are from users clicking on an email - we will be moving it to a more modern one cost w/offsite backup is few $k per year, slowed down radio link for first initial backup
mailing list requests
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There is no open time left in Q3.Looked for opportunities to reduce M3 rotations but there weren't a lot because we didn't find many. But we are getting faster at doing it in person. Had one ToO call last night; payback date will be updated in next Q3 update.
Schedule in progress, might be ready in a couple days. Monitoring programs coming back (Q4, Q1), quarter night programs adjacent to each other. Fine when last 2 quarters of night, so other programs have lots of shares. 7 different programs doing partial night observers. Some 1-2hrs at beginning or end. Fewer very flexible programs to pad those. Hoping teriaty rotations will be faster. If you think start/end times are wrong let us know. Packed so efficiently that we'll have several open bright halves for people to request. Also have several classes (4) and another visiting instrument run back to back
Aleksandr - Mike Joner is scheduled soon and the filter wheel is broken and we don't have an estimate for when it would be fixed but we need to tell him soon. He can choose to observe with no filter or request time later on. Hopefully have answer about wheel before sending out call
Open action items from previous meetings:
New action items from this meeting:
High speed imaging -is MBASIC still on the table? multi-bad
The next meeting will be on October 3 at 10:30 MDT.