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A Photometric System to Search for Optical Variability on Time-scales of 3 x 10-7 to 300s: Main Results

Published online by Cambridge University Press:  12 April 2016

G.M. Beskin ,
S.I. Neizvestnyi ,
A.A. Pimonov ,
V.L. Plakhotnichenko  and
V.F. Shvartsman
G.M. Beskin
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Stavropolskij Kraj 357140, USSR
S.I. Neizvestnyi
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Stavropolskij Kraj 357140, USSR
A.A. Pimonov
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Stavropolskij Kraj 357140, USSR
V.L. Plakhotnichenko
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Stavropolskij Kraj 357140, USSR
V.F. Shvartsman
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Stavropolskij Kraj 357140, USSR

Extract

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One of the basic astrophysical problems is to search for and investigate brightness fluctuations of celestial objects at times comparable with the mean time between registered photons. With that end in view, a special mathematical formalism has been developed in recent years (Shvartsman, 1977; Pimonov and Terebizh, 1981; Plakhotnichenko, 1980).

Type
Section II: Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 67: Instrumentation for Astronomy with Large Optical Telescopes , 1982 , pp. 181 - 184
Copyright
Copyright © Reidel 1982

References

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