Semester
The table below summarises the classically-scheduled programs that have been awarded time on Gemini North and South, as well as programs from the Gemini community awarded Exchange time on Subaru. Jump directly to the schedule for:
Each Gemini program has been assigned a Contact Scientist (CS) who is the point of contact between the Observatory and the Principal Investigator. Instructions for visiting observers are available.
The columns in the table are:
Date: Scheduled observing night(s), local time, for the Gemini telescopes, or number of nights and preliminary dates for Subaru.
Allocated programs: Gemini reference number, Principal Investigator and Partner.
Instrument: name of the instrument(s).
Title: the title of the program.
Classical programs scheduled for Gemini South in .
| Schedule : Gemini South | |||
| Date (Local Time) and Award | Allocated Program | Instrument | Title |
TBD |
GS-2025A-C-1 Cassanelli, AR, CA, CL, US | Iqueye |
Iqueye at Gemini South: the highest sensitivity to look at the fastest variable astronomical objects |
Classical/Queue programs scheduled for Subaru in . See the Subaru Schedule to confirm dates.
| Schedule : Subaru | |||
| Award, date(s) | Allocated Program | Instrument | Title |
|
2/18(1st)+3/8(1st), 0.5n |
S25A-TE009-G, Jiang, CA |
VAMPIRES |
Confirming the direct detection of a runaway accreting protoplanet |
|
2/23-26 (2nd x 4) + 4/23(1st), 2.5n |
S25A-TE028, Hudson, CA |
HSC |
Extending the UNIONS g-band |
|
6/5(1st), 0.5n |
S25A-TE013-G, Bhangal, CA |
MOIRCS |
MOIRCS study of a protocluster core in H-alpha at z = 2.3 |
|
0.5n, Queue Grade-B |
S25A-TE005-GQ, Cho, KR |
HSC |
A Large-scale Cosmic Filament Aligned with Galaxy Cluster Merging Axis: A Dark Matter Perspective |
|
0.732n, Queue |
S25A-TE092-GQ, Monteiro-Oliveira, US |
HSC |
Mapping the dark matter distribution in highly massive merging clusters newly discovered by eROSITA |
|
0.5n, ToO |
S25A-TE194-G, Polin, US |
FOCAS |
Investigating the Origin Calcium Strong Transients |