- Type = Object type:
- Point Source: stars & QSOs
- Galaxy: distant compact sources - seeing dominated profile
- Nearby Galaxy: distant compact sources - object dominated profile
- Extended Source: uniform illumination over square arcsecond scales
- Filter = Bandwidth selection:
Only the B,V,R & I filters are supported but using the level
sky field entry, one can constraint DIET to compute numbers
for other filters.
- Mag. = Object magnitude:
Magnitude of the object, or class of objects, to observe.
- SNR = Signal-to-noise ratio on the object:
The signal-to-noise ratio of the object, or class of objects, to achieve
for the magnitude defined in the previous field. Here are typical values required
depending on the scientific program. Refer to the documentation for a complete
discussion on the subject.
- SNR = 3 : Detection - Photometry error = 33%
- SNR = 7 : Fair detection - Photometry error = 15%
- SNR = 15 : Good detection - Photometry error = 7%
- SNR = 25 : Quality photometry - Photometry error = 4%
- #Night = Number of nights for the program:
The maximum number of nights available can be imposed. If the total exposure
time computed by DIET exceeds what can be achieved in the maximum available time
including all nights (assuming an object that would go through zenith in the
middle of the night
- #Night = Auto :
- #Night = {1,2,3,4} :
- Seeing = Image quality:
- Sky = Sky brightness:
- Airmass = Median airmass of the observation:
- %Atm.Tr. = Atmosphere transparency:
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