blog:20231119

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20231119

1515-

Roy, Olivia

PHYS 401, 433C, Dome

  1. Reattach 432 to DFM Scope with Filter Wheel
  2. Collect Calibration Frames
  3. Monitor in-dome and ambient temperatures to support understanding seeing measurements
  4. Collect data for limiting magnitude study
  5. Review Data Redux Pipeline
Time Observed Source Name Filter Int Time [s] Mag (filter) RA [h] DEC [deg] Source Type Scope Purpose Notes DomeTemp [C]
YYYYMMDDThhmm (HD/NGC/ETC) UVBRI e.g., 3 1.25(V) 20 45 Star Main Pointing 15.042 w/o ag 14
  1. Opened dome at 1515
  2. Turned-on exhaust fan
  3. Attached 432 to UVBRI Filter Wheel to Instrument Rotator to GAM-lite
  4. Taped Icron LED lights up and taped gap above instrument rotator (see picture)
  5. Choosing not to North-align to favor collection of sky flats
  6. Set focus to 1907.4, which was the optimal focus arrived at on 20231117
  1. Sky Alert Data file uploaded to 2023-11-19 file on gDrive
  1. All frames copied to 2023-11-19 on gDrive