||P60: 20191001 - 20200401
||Daniele Malesani, Silvia Piranomonte
||Why NOT? Discovering and characterizing optical counterparts of gravitational wave sources.
||Discovery 20 targets, 5min/target, 10 nights 1.2h/nt follow-up
|| Can also override time-critical programs! 5 triggers over 3 semesters
|Total Time Spent
Hard ToO:02:33 Soft ToO:
||AT2019wxt, SP0305+261, AT2019wxt
||ALCl180060 - ALCl180068, ALCl180069 - ALCl180074, ALCl180075 - ALCl180078, ALCl180081 - ALCl180084
||Targets successfully observed. Weather was good for the spectroscopic part, but
there were some upper cirrus while taking the images both times when this was
attempted (20:40 and 02:05 UTC). DIMM seeing between 0.8 and 1.0 arcseconds
at the beginning of the night, and 1.1 while imaging for the second time. No issues
||ALDc120070 - ALDc120084
||Target was observed through thin clouds with seeing around 1.3 arcsec. The standard was observed
immediately after the target.
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