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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.
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