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Photometric Monitoring of Selected Quasars: The Highly Luminous Quasar HS 1946+7658

Published online by Cambridge University Press:  25 May 2016

B.M. Mihov ,
R.S. Bachev ,
A.A. Strigachev ,
L.S. Slavcheva  and
G.T. Petrov
B.M. Mihov
Affiliation:
Institute of Astronomy, 72 Tsar, chausse Blvd., 1784 Sofia, Bulgaria e-mail: bmihov@astro.bas.bg
R.S. Bachev
Affiliation:
Institute of Astronomy, 72 Tsar, chausse Blvd., 1784 Sofia, Bulgaria e-mail: bmihov@astro.bas.bg
A.A. Strigachev
Affiliation:
Institute of Astronomy, 72 Tsar, chausse Blvd., 1784 Sofia, Bulgaria e-mail: bmihov@astro.bas.bg
L.S. Slavcheva
Affiliation:
Institute of Astronomy, 72 Tsar, chausse Blvd., 1784 Sofia, Bulgaria e-mail: bmihov@astro.bas.bg
G.T. Petrov
Affiliation:
Institute of Astronomy, 72 Tsar, chausse Blvd., 1784 Sofia, Bulgaria e-mail: bmihov@astro.bas.bg

Abstract

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We present and discuss Johnson – Cousins V and R photometry of the highly luminous quasar HS 1946+7658 (z = 3.051). We found no evidence for strong variability during one year of monitoring.

Type
II. Observational Properties of AGN and Related Objects
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 175 - 176
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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