blog:20250601

20250601

2230

Dylan Williamson, Percy Yu, Jason Fischer, Ian Kirn

401, Control room, dome

1. Train Jason and Dylan on Astropol procedures: changing the camera, data management for the PICSI2 2. Astropol data 3. Implement the “north up” procedure before taking captures

https://docs.google.com/document/d/1KBDuFkNJU6Wv7AL-5MnjEbJ2MCA1C602ObkQQ6Y2NNg/edit?usp=sharing

Scope Camera Focus
MainPICSI2 w/ ASI 5332600
FinderASI 4322465
Time Observed Source Name Filter Int Time [s] Gain Airmass Mag (filter) RA [h] DEC [deg] Source Type Scope Purpose Notes
YYYYmmddTHHMM Object Filter time gain airmass mag(V) HH DD type Scope Purpose tracking? Others?
  • 2230 Ian sets up the dome with Dylan and Jason
  • 2240-1230 Fixing detector orientation to “north up” and Ian demonstrated how to put on the detector
  • 0100 Ian leaves
  • 0128 3C 273 was not viable, too low
  • 0130 Clouds rolled in
  • 0142 Slewed to Vega to confirm that there was no pointing error, cloud cover making it difficult to see high magnitude targets
  • 0150 Skipping TON 599 and 3C273 captures due to the high sky cover, and going down to where AM Her observations begin
  • 0230 Slewing to BL Lac as requested by Ian. Will be observing Bl Lac as the main target for the rest of the night. Calibration targets will remain the same

Astropol is implementing a technique to ensure that the detector is “north up” - to decrease the amount of drift that occurs during long exposures. If not “north up”, the RA tracking movements can “leak” into the DEC, and move the target vertically on during captures.