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- W2029730047 abstract "Approximate signal-to-noise ratios are calculated for 12 stellar occultations by the rings of Uranus during 1977-1980. Four of the stars are apparently bright enough to permit observation of the epsilon-ring occultations with a large telescope. For the best of these events, occultations by rings alpha through delta should also be observable with a large telescope, and epsilon-ring occultations should be detectable with smaller telescopes. Formulas for the signal-to-noise ratios are given to aid potential observers in evaluating the quality of the results they can expect to obtain with their own photometric equipment." @default.
- W2029730047 created "2016-06-24" @default.
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- W2029730047 date "1977-12-01" @default.
- W2029730047 modified "2023-09-27" @default.
- W2029730047 title "Signal-to-noise ratios for stellar occultations by the rings of Uranus, 1977-1980" @default.
- W2029730047 doi "https://doi.org/10.1086/112166" @default.
- W2029730047 hasPublicationYear "1977" @default.
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