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
Time Observed Source Name Filter Int Time [s] Mag (filter) RA [h] DEC [deg] Source Type Scope Purpose Notes DomeTemp [C]
20231119T1625 FLAT U 0.08s - - - FLAT Main Calibration Used NINA 14
20231119T1703 FLAT B 0.21s - - - FLAT Main Calibration Used NINA 14
20231119T1703 FLAT V 0.21s - - - FLAT Main Calibration Used NINA 14
20231119T1703 FLAT R 0.10s - - - FLAT Main Calibration Used NINA 14
20231119T1703 FLAT I 0.11s - - - FLAT Main Calibration Used NINA 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
  7. Took flats while sun was setting, had to move towards west because of moving object in frames
  1. Sky Alert Data file uploaded to 2023-11-19 file on gDrive
  1. All frames copied to 2023-11-19 on gDrive