Observers: Sun Mi Chung, Michael Fausnaugh, Loreto Barcos-Munoz SA: Dave T. TO: Steve A. Summary: Light to moderate cirrus throughout the entire night. Seeing started off at ~1.1 arcsec, then jumped to >1.5 arcsec, then back down to ~1.3 arcsec. Started with MODS, then switched to LBC for the last few hours of the night. Completed programs in MODS: UM_Novae/EG131_5.0, UM_Novae/1974cyg_0.8, UM_Novae/1974cyg_5.0, Uva_BCD/J2104, Uva_BCD/0045AGN (*this program received double the requested time because seeing jumped up to ~1.7 arcsec and clouds moved in*. Seeing eventually improved and stabilized ~1.2 arcsec), and OSU_MAP/IC0342. Two flux standards also completed -- BD284211 and gd121. Completed programs in LBC: OSU_Monitor/N672, OSU_Monitor/N628, OSU_Monitor/925 ********************************************************** Afternoon calibrations: 10:00 Calibrations for LUCI (programs from 1026) and MODS (for 1027) 10:30 Partly cloudy, more on the way.... MODS: 12:40 Sunset. Moderate cloud coverage, especially near horizon 01:11 Start acquisition on BD284211 standard 01:20 Start observation on standard star. Note we are still in twilight. Seeing ~0.9 arcsec 01:32 Another set of 3 exposures on standard star BD284211. 01:42 Preset to UM_Novae/EG131_5.0. Start acquisition. 01:50 Acquisition image shows collimation problems -- the "rabbit ears". Continue with acquition. ** NOTE: The "rabbit ears" effect seen in very bright stars is a known PSF artifact of the rigid secondary - also known as the "evil space bunnies" artifact. It is not a consequence of poor collimation. It will be visible in all MODS and LUCI images of very bright stars even with perfect collimation, as well as showing fine structure in the "ears" during episodes of exceptionally good seeing. [rwp/osu] 01:52 Start observation on UM_Novae/EG131_5.0 *** 01:58 Twilight ends ***** 02:01 Preset to UM_Novae/1974cyg_0.8, start acquisition. 02:10 Two nearly equally bright sources. Cannot identify which is the target -- insufficient finding chart! Clarified with PI on the phone. 02:19 Start observation. Seeing ~1.1 02:41 Start acquisition on UM_Novae/1974cyg_5.0. 02:49 Start observation on 1974cyg_5.0. Seeing is ~1 arcsec 03:11 Starting acquisition on UVa_BCD/J2104. Clouds on horizon. Seeing: ~1.0" 03:25 Starting observation on UVa_BCD/J2104 04:15 Starting acquisition on UVa_BCD/0045AGN. Seeing ~1.3" Guide star wasn't recognized because it is not a star! 04:24 Modify script -- change the position angle from 0 to 180 (i.e. slit is still in the same direction) and choose a new guide star. 04:27 Start acquisition on the modified script with the new guide star. 04:41 Start observation on UVa_BCD/0045AGN. Seeing ~1.2" Light cirrus. 05:00 Seeing is worse, ~1.5 to 1.7. Cloudy. 05:29 Rerunning UVaBCD/0045AGN, since seeing is higher than desired. 05:40 Seeing is somewhat improved, seems stable around ~1.2 to 1.4 06:18 Starting acquisition for standard star, gd191 06:28 Starting observation of gd191 06:40 Starting acquisition on OSU_MAP/IC0342 06:54 Start observation on IC0342. Seeing is ~1.3 07:09 Seeing is better ~1.1 07:17 Seeing is ~1.3 07:48 Seeing is 1.1 08:18 Seeing is ~1.4 08:49 Seeing is 1.1 ******* 09:13 START SWITCHING TO LBC ************** LBC: 09:46 Send preset to OSU_monitor_N628_focus field 09:49 Start collimation with dofpia. Note, more cirrus rolling in. 10:11 co-pointing correction with lbcrangebal 10:13 Start OSU_monitor_N628 science OB. Moderate cirrus. FWHM in blue 1.4 arcsec, FWHM in red 0.9 arcsec Blue point sources appear elongated. 10:33 FWHM in red 1.1 arcsec 10:49 Send preset to OSU_monitor_672_focus field 10:51 Start collimation on focus field 10:53 Start co-pointing 10:58 Start science OB for OSU_monitor_672. Moderate cirrus 11:08 Seeing is 0.9 arcsec in blue and red 11:34 Send present to OSU_monitor_925_focus field 11:35 Start collimation on focus field 11:40 Start science OB for OSU_monitor_925. Moderate cirrus. 11:51 Seeing is 0.7 arcsec in blue and red. Still moderate cirrus. 12:07 Re-run science OB for OSU_monitor_925, since we have nothing else to observe for the remaining ~10 minutes before twilight. Last few exposures saturating in red. Start testing twilight flat counts. 12:30 -- Twilight flats in blue Uspec, B, V, and red R filter.