Search
Text Size:
Smaller Text Normal Text Larger Text

Facebook page

Twitter profile

YouTube channel

70-205 Pursuing the first lights from core-collapse supernovae: rapid follow-up observations of Einstein Probe alerts

PI: David Aguado

Observing instructions:

Go to the directory
  cd ~/scripts/70-205

execute the requested scripts. CAN ONLY TRIGGER ON CAT NIGHTS!

Program Tracking
Proposal 70-205
Semester P70: 20241001 - 20250401
Principal Investigator Aguado
Programme Pursuing the first lights from core-collapse supernovae: rapid follow-up observations of Einstein Probe alerts
Instrument ALFOSC
Time Allocation Max 10 tiggers of 1 hour each
Total Nights
Type ToO
Notes Only allowed to override CAT service and CAT visitor nights
Total Time Spent 02:20 (hh:mm)   Hard ToO:02:20   Soft ToO:
Proposal Date Time Type Targets Files Comments Status
70-205 2024-11-22 00:50 ToO EP241021a Sky flats were taken during twilight. Focus just before observations (lower hatch closed) Seeing around 2 arcsec Script ep241021a_bis_ep241021a_r_nov launched at 21:50; observations started around 21:50 and finished at 22:40. Seeing improved slightly.Wind gusts though the observation. Observed
70-205 2024-11-26 00:00 ToO Clouds entered around 2am preventing the observations. Failed
70-205 2024-12-13 00:00 ToO Very cloudy all night Failed
70-205 2024-12-18 00:00 ToO Target could not be observed tonight as ALFOSC was not mounted Failed
70-205 2024-12-27 01:00 ToO SN2024aecx Calibrations were done following ALFOSC coockbook for the 0.5" slit. The observing block prepared by the PI of 70-205 was completed, without changing the slit size (0.5"). Despite bad seeing conditions (~3 arcsec), the SN was clearly seen. Observed
70-205 2025-01-07 00:30 ToO SN2024aecx ALIa070141 - ALIa070144 SN2024abfo could not be observed due to clouds. SN2024aecx observed with sub-arcsecond seeing. For future triggers, please submit different transients as different groups - OB generator help states: A Group consists of all observations which _need_ to be executed in a single night (e.g., an object and a standard star). Observed

 

The above information is collected from the ToO/Mon reports that have been created by the observer.

Should any of the observations have been carried out using the OB system, you will find additional information HERE

Back to top Last modified: September 16 2024