Subject: 3.5m Night Log 20181028 From: cgray@apo.nmsu.edu Date: Mon, 29 Oct 2018 12:50:51 +0000 (UTC) Apache Point Observatory 3.5m Telescope Night Log Sunday, October 28, 2018 ACTUAL ASTRONOMER OBSERVER(S) INSTRUMENT START FINISH -------------------------------------------------------------------- Y.Zhu D.Ren, X.Zhang PAO 18:24 06:47 INST SCHEDULED WEATH EQUIP OBS NOT USED I/ROW/DN START FINISH D B D B D B D B ---------------------------------------------------------------- NI01/O 18:24 07:10 0 0 0 0 3.3 9.4 0 0 note: scheduled times listed include instrument change time ------------- ACTIVITY LOG -------------- Observing Specialist: C.Gray There will be no foolish mounting or silly counter-rotations in this dome. As such, Russet does not expect many of us to appreciate the subtle science and exact art that is a visiting instrument. However, for those select few who possess the pre-assigned shift, she can teach us how to bewitch the night and ensnare the photons. She can tell us how to bottle fear, brew coffee, and even put a stopper in the light path. Then again, there are some of us that have come to APO in possession of abilities so formidable that we feel confident enough to not pay attention. However, Russet will remind us that it takes a great deal of bravery to stand up to your friends, but a great deal more to stand up to your visitors. The PAO is here on a clear, subarcsecond night and I see that they, like many before them, have discovered the delights of the Mirror of the 3.5m. I trust by now they realize what they can do. The clearest star in the sky would look into the PAO and see itself, exactly as it is. The PAO shows us nothing more or less than the deepest and most desperate desires for a calm sky. But remember this, the 3.5m mirror gives us neither clear sky or good seeing, and thin clouds rolled in near midnight and were here to stay. There will come a time when the PAO must be told something. But I must wait until the team is at their most fatigued. On the night the PAO went to the NA2 to collect photons, and the lenslets cast itself between them, the light rebounded. When that happened, a part of the sky latched its onto the only recording thing it could find. The imager itself. But there's a reason the stars are fluttering in the sky. That's a reason they are becoming fainter. The light of the dawn is coming inside the dome. So, when the time comes, the dome must close. Yes, yes it must close. We've kept things open so that we can close at the proper moment. We've been tracking the sky up and our sleep has been slaughtered. Though don't tell me now that I've grown to care for such nights. Close...after all this time? Always. I solemnly swear that I am up to no good. Even so, no problems tonight. ------- FAILURE LOG ------- PROG INST FAILURE MODE TIME (SEDFNVOG) TI/SHU START FINISH DESCRIPTION ---------------------------------------------------------------------- ---------------- FOCUS LOG --------------- Time Instrument Focus Az El Temp Strc Prim Sec Air filt FWHM -------------------------------------------------------------------------- 18:46 pao 135( -876) 123 59 10.9 11.5 11.3 11.2 10.1 -- 1.21 21:33 pao 110( -977) 9 61 9.9 10.1 10.6 9.4 9.4 -- 0.80 ------------- WEATHER LOG ---------------- Wind Precip.or Time Temp F Dewp F MPH Direction Dust Sky Conditions ------------------------------------------------------------------ 16:00 57 34 5 343 (NNW) 82 clear none 17:00 55 31 8 308 (NW) 82 clear none 18:00 52 27 3 347 (NNW) 84 clear none 19:00 52 8 6 347 (NNW) 7 clear none 20:00 52 13 3 350 (N) 0 clear none 21:00 53 9 6 352 (N) 3 mstly clr none 22:00 51 12 3 337 (NNW) 5 mstly clr none 23:00 51 19 6 293 (WNW) 0 mstly clr none 00:00 50 21 3 280 (W) 1 mstly clr none 01:00 47 29 2 340 (NNW) 1 mstly clr none 02:00 51 26 1 350 (N) 2 mstly clr none 03:00 51 23 5 273 (W) 0 ptly cldy none 04:00 50 26 5 288 (WNW) 3 ptly cldy none 05:00 47 33 3 214 (SW) 4 mstly clr none 06:00 48 25 3 191 (S) 1 mstly clr none Note: the wind was coming from the azimuth listed. The convention used is north=0 degrees, east=90 degrees. The dust count is particles > 1u per 0.1 cubic feet. TELESCOPE STATUS Telescope drives operational. Current TCC version: 1.2.4 Current TUI version: 2.6.0