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- W2022112296 abstract "A discussion is given of experience gained at the Radcliffe Observatory during the past five or six years in the use of the Fabry method of stellar photometry. An accurate light curve of the eclipsing variable RS Sgtr has been determined by this means. The average deviation from the mean light curve for one exposure was 0 m .013. Experiments have been made to observe by continuous recording, instead of by discrete exposures, but little improvement of accuracy has so far been achieved, except on nights with a poor sky. Results obtained in checking a magnitude sequence in Harvard Standard Region E3 are given, and compared with four sets of independently determined magnitudes. Of the five sets of measures, those made by the Fabry method show the smallest average deviation from the mean." @default.
- W2022112296 created "2016-06-24" @default.
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- W2022112296 date "1945-08-01" @default.
- W2022112296 modified "2023-09-27" @default.
- W2022112296 title "The Fabry Method of Stellar Photometry" @default.
- W2022112296 doi "https://doi.org/10.1093/mnras/105.4.212" @default.
- W2022112296 hasPublicationYear "1945" @default.
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