Date: Thu, 25 Feb 1999 06:34:53 -0700 (MST) From: Russet McMillan Subject: 3.5m Night Log 990224 Apache Point Observatory, Sunspot, NM Wednesday, February 24th, 1999 3.5-meter Night Observing Log Actual ---------------------------------------------------------------------- ASTRONOMER OBSERVER(S) INSTRUMENT DATE START FINISH ---------------------------------------------------------------------- C.Stubbs C.Hastings SPIcam 2/24 19:18 20:08 D.Leeber D.Leeber GRIM II 2/24-25 20:28 05:14 ---------------------------------------------------------------------- INST SCHEDULED WEATH EQUIP OBS DAY NOTUSED I/RS/DN START FINISH D B D B D B USE D B ---------------------------------------------------------------------- EN02/S 19:18 20:18 - 0 - 0 - 1.0 0 - 0 NM05/S 20:18 05:14 0 0 0 0.3 2.2 6.5 0 0 0 -------------- Activity Log -------------- 1st Half Observing Specialist: N.C.Hastings We opened at 16:30 for cooling. Dale had GRIM back on line for tonight's program and it seems to be behaving well. I was the observer for the UW program, and clouds hindered us all night. Dawn Leeber was on site to observe for NMSU. The seeing monitor was also set up tonight by APO staff, myself. We had a two errors with file writing that were easily corrected. Observing went smoothly and only the clouds interfered. 2nd Half Observing Specialist: R.McMillan After NM05's main object of interest had set, with cirrus preventing accurate photometry, they decided to switch to DIS. In the process, we discovered that the calibration lamp controls had not survived the LAN switchover on Saturday. Since the purpose of the spectroscopy was just to do spectral classifications, the observer elected to continue using DIS even without arc lamps. Interesting note: DIS apparently dumped its nitrogen while it was mounted, because at dawn it was 20 lbs lower than usual for that time of day. But it didn't dump *all* its nitrogen, and it didn't warm up. This could be consistent with the theory that the dumps occur when the instrument is at some undesirable rotation during one of the scheduled fills. Tonight, the second half program included many short exposures on bright stars -- so perhaps DIS moved either to or from that undesirable rotation value in the middle of a fill. If my calculations are correct (using the fill time obtained through "dis ln2 status"), the fill started at 03:49. OBSERVER COMMENTS T.Harris (NM05): Given the appearance of the weather at sunset, it is surprising that we were able to observe all night. Dawn Leeber used GRIM to observe V616 Mon for the first half of the night. Due to the cirrus, we decided to switch to DIS since our second half objects needed photometry. We observed 17 different objects with DIS and obtained excellent spectra. FOCUS LOG February 24th 1999 Best Telescope Temp Wind Seeing Time Instrmnt Focus Az El Air/Truss Dir MPH filter FWHM" --------------------------------------------------------------------- 18:55 SPIcam -250(6120) 092 46 3.6/5.8 268 09 V 1.59" 19:02 Guider 52000(6077) 093 47 3.6/5.7 263 06 none 1.64" 20:28 GRIM II -180(6236) 190 56 4.9/4.9 234 09 J-f/5 0.72" 01:45 DIS -200(6132) 186 57 5.3/5.0 290 23 Gunn 0.94 WEATHER LOG February 24th 1999 Wind Time Temp-F Dewp-F MPH Direction Dust Sky Precip ------------------------------------------------------------------ 16:01 48 5 10 269 (W) 823 mstly cldy none 17:01 43 1 8 315 (NW) 806 mstly cldy none 18:01 41 0 5 281 (W) 913 ptly cldy none 19:01 38 -2 8 267 (W) 810 cirrus none 20:01 41 0 6 264 (W) 817 cirrus none 21:01 41 0 9 221 (SW) 711 cirrus none 22:01 41 0 9 228 (SW) 894 cirrus none 23:01 42 0 8 265 (W) 756 cirrus none 00:01 42 0 14 273 (W) 648 cirrus none 01:01 42 0 15 264 (W) 600 cirrus none 02:01 42 1 16 273 (W) 589 cirrus none 03:01 42 1 20 284 (WNW) 555 cirrus none 04:01 42 1 18 280 (W) 536 ptly cldy none 05:01 42 0 16 269 (W) 637 mstly cldy none 06:01 42 1 12 268 (W) 617 mstly cldy none note: the wind was coming from the azimuth listed. The convention used is north=0 degrees, east=90 degrees. The dust count is for the particles > 1 micron per 0.1 cu.ft. TELESCOPE STATUS Primary, secondary, and tertiary mirrors in place and collimated. Primary support system operational. Mirror ventilation system in place. Telescope drives operational. Current Remark version: 2.54b4 Current guide software version: GIm Ctrl v3.0b 17.out - NCH, RM