Department of Physics AstroLab

Exposure Time Calculator

Magnitude:

Seeing ("):

Zenith Angle (deg):

Exposure Time (s):

Filter:

Telescope:

Sky Background:

Cloud Cover:

This webpage calculates an estimate of the total counts, peak counts and signal to noise ratio, if a star was observed for the conditions specified. The SNR should be maximised but without exceeding the detector's linearity limit.


Expected magnitudes are approximately 7-18. Typical seeing conditions are 1-5 arcseconds. The zenith angle is measured downwards from the zenith with the horizon at 90 degrees. The sky background level is dictated predominantly by the position and phase of the moon.