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Long-term monitoring of a large sample of active galactic nuclei

  • Alex G. Smith
  • R. J. Leacock
  • J. R. Webb
III. Optical Variability Studies
Part of the Lecture Notes in Physics book series (LNP, volume 307)

Keywords

Light Curve Light Curf Active Galactic Nucleus Period Find Strong Period 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Babadzhanyants, M.K. and Beloken, E.T. (1984). Astrofizika 21, 231.Google Scholar
  2. Barbieri, C., Romano, G., di Serigio, S., and Zambon, M. (1977). Astron. and Astrophys. 59, 419.Google Scholar
  3. Bevington, P.R. (1969). Data Reduction and Error Analysis for the Physical Sciences (McGraw-Hill).Google Scholar
  4. Pollock, J.T., Pica, A.J., Smith, A.G., Leacock, R.J., Edwards, P.L. and Scott, R.L. (1979). Astron. J. 84, 1658.Google Scholar
  5. Smyth, M.J. and Wollstencroft, R.D. (1970). Astrophys. and Space Sci. 8, 471.Google Scholar
  6. Webb, J.R., Smith, A.G., Leacock, R.J., Fitzgibbons, G.L., Gombola, P., and Shepherd, D.W. (1988). In the press, Astron., J., Feb. 1988.Google Scholar

Copyright information

© Springer-Verlag 1988

Authors and Affiliations

  • Alex G. Smith
    • 1
  • R. J. Leacock
    • 1
  • J. R. Webb
    • 1
  1. 1.Department of AstronomyUniversity of FloridaUSA

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