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- W1630689967 abstract "Abstract The appearance of SN 1987A led to the implementation of a fast sampling option in the data collection system of the photometer on the University of Tasmania’s optical telescope. This option permits acquisition of continuous data trains of over one hour’s duration at sample rates of 5 kHz. Monitoring of SN 1987 A at regular intervals has permitted upper limits to be assigned to any pulsed fraction of the optical flux. Successful test observations of the Crab pulsar have been obtained, as well as observations of the geostationary Aussat satellites during their bi-annual specular-reflection episodes. For the latter, very accurate spin rates (∼1 Hz) are determinable in short data runs because of the higher frequency components (∼100 Hz) in their light curves. These components are produced by the rows of solar cells on the outer surfaces of the satellites, and fast-Fourier transform analyses essentially permit the numbers of rows of cells to be counted precisely." @default.
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- W1630689967 date "1989-01-01" @default.
- W1630689967 modified "2023-09-24" @default.
- W1630689967 title "Fast Photometry of the Crab, SN 1987A and Aussat" @default.
- W1630689967 cites W2004329219 @default.
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- W1630689967 doi "https://doi.org/10.1017/s1323358000022955" @default.
- W1630689967 hasPublicationYear "1989" @default.
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