How much more time do you need from a bright site?
Compare two observing sites by SQM reading to see how integration time trades off against sky brightness, adjusted for your target and filter type.
Inputs
Results
Adjust the inputs to see results.
Pogson magnitude scale (N. Pogson, 1856): brightness ratio = 10^(0.4 × ΔSQM). Adjusted for target/filter sensitivity.
All formulas verified by automated tests.