The table below summarizes the amount of time each program has
used.
Program is the observing run name, or the coversheet
identification. "public" is a special observation, where the data are
available to all users. These are generally standard star
observations. Other examples may include pointing models which are
not charge to any one and do not have any corresponding exposure time.
The value in the Obs, for observation time, is the total number
of hours of clock time including overhead used by the program.
The value in the Exp column, for exposure time, is the total
number of hours of open shutter time for that program.
Alloc is the allocation to the program by the TAC in hours.
Team simply lists the program team, with the subitting PI first.
Program
Obs(hr)
Exp(hr)
Alloc(hr)
Team
2024A_A000i0
0.84
0.80
10.00
Metevier/Sakari/Shetrone
2024A_A001i0
3.12
2.77
30.00
Holden/Dressing/Isaacson/Kane/Luhn/Robertson/Burt
2024A_A002i0
0.30
0.02
20.00
Kane/Isaacson/Fulton
2024A_A003i0
5.08
4.70
90.00
Lu/Lam/Simon/El-Badry
2024A_A006i0
2.02
1.84
32.50
Hill/Kane/Fulton
2024A_A008i0
10.71
10.15
20.00
Konopacky/Baburaj/Theissen/Hoch
2024A_A009i0
10.38
9.54
25.00
Lubin
2024A_A010i0
3.73
3.40
10.00
GuhaThakurta/Chakrabarti/Simon
2024A_A012i0
8.00
7.30
70.00
Lu/Rowan/Abrams
2024A_A013i0
7.33
6.47
169.00
Luhn/Robertson/Isaacson/Holden
2024A_A014i0
5.94
5.49
50.00
Melis
2024A_A015i0
0.42
0.39
60.00
Shetrone/Sakari/Tang/Carrasco
2024A_A017i0
9.52
7.68
100.00
Howard/Fulton/Isaacson
public
0.00
0.00
total
67.39
60.57
Conditions Summary Table
This table simple summarizes the observing conditions per month.
Month is the year, month and starting day of the time considered.
Total represents the total number of hours of darkness, defined
as between -9 degree sunset to -9 degree sunrise, over the month.
OK gives the number of hours it was determined to be ok to open
the telescope. Reasons for closure may include weather or
engineering issues.
The FWHM lists the average seeing for the month.
Transparency lists the typical transparency for the telescope in
magnitudes as compared to a fiducial zeropoint. This may reflect
clouds or it may reflect other issues.