OSURC run, night 3: UT October 25, 2019

Observers:
   Charlotte Wood, University of Notre Dame du Lac
   Donald Terndrup, The Ohio State University

LBTO Astronomer:
   Olga Kuhn

Telescope operator:
   Josh Williams

Clear at the start of the night.  Seeing is very poor, 1.7" - 1.9"
at opening and was only better occasionally.  We thus began with 
bright AGN as part of the OSU_Storm program.  During periods when
the seeing was somewhat less bad, we got a couple of programs from 
the main list.

Completed programs:
  OSU_Storm: PG 2130, Mrk 335, Mrk 1501, NGC 7469,
             PG 0026, PG 0052
  OSU_dwarfs/NGC628A
  UVa_UVA_BCD_J0344
  OSU_ASASSN/ZTF19abvgxrq
    
Afternoon: calibration images
   slit flats: 0.6", 0.8", 1.0", 1.2"  dual mode

Morning: calibration images (more tomorrow)
   Lamp spectra Mods1 (red) + Mods2 (blue)
   slit flats: 2.4"   dual mode

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UT_start  Object/Notes

  01:30   BD+28 4211 dual mode
          Seeing 1.5 - 1.6"

  01:40   BD+28 4211 mods1: red  mods2: blue
          This is the configuration for the OSU_Storm project
          Seeing 1.5"

  02:05   OSU_Storm/PG2130
          Seeing 1.5"

  02:45   OSU_Storm/Mrk335
          Seeing 1.3 - 1.6" (range indicates variability)

  03:25   OSU_Storm/Mrk1501
          Seeing 1.7 - 2.0"
  
  04:05   OSU_Storm/NGC7469
          Seeing 1.3 - 1.5"  

  04:50   OSU_Storm/PG0026
          Seeing 1.5 - 1.8"

  05:25   OSU_Storm/PG0052
          Seeing 1.8", but improved during the sequence

  05:55   Go to OSU_dwarfs NGC628A field.  DIMM 1.65"
          Centered on the target galaxy, assume slit rotation is correct
          to get the companion dwarf to the southwest.  Had to make a
          few corrections to the acquisition file (slit image name
          incorrect).  Seeing on acquisition images: 1.6" (red), 1.85" (blue)
  06:15   Begin sequence.  Seeing is improving while we are observing.
          Object is extremely faint. Targeted object does not have any
          obvious spectral features. Companion galaxy to the south 
          shows definite emission lines with an approximate redshift of 0.026
          (Balmer alpha + beta + [O III] + [O II]). 

  07:25   Move over to UVA_BCD_J0344.  DIMM 1.5".
  07:35   Start spectra.  Seeing variable, sometimes good, often not.

  08:45   Set up on OSU_ASASSN/ZTF19arglebargle.  This is a second epoch.
          Seeing is pretty crappy, but we'll try anyway.
          We did the observing sequence twice because the seeing 
          was sometimes about 2" and the light through the slit was reduced.

  11:30   g191b2b dual mode
  11:50   g191b2b mods1: red  mods2: blue

  12:10   gd71 dual mode, then    mods1: red  mods2: blue

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