Astron. Astrophys. Suppl. Ser. 134, 453-461
R. Sagar1,2 - Gopal-Krishna3 - V. Mohan1 - A.K. Pandey1 - B.C. Bhatt1,2 - S.J. Wagner4
Send offprint request: R. Sagar, Naini Tal
1 - U.P. State Observatory, Manora Peak, Naini Tal, India
e-mail: sagar@upso.ernet.in
2 -
Indian Institute of Astrophysics, Bangalore 560034, India
3 -
N.C.R.A.-T.I.F.R., Pune University Campus, Pune-411007, India
4 -
Landessternwarte Heidelberg-Koenigstuhl, 69117 Heidelberg, Germany
Received July 28; accepted August 31, 1998
We report multi-colour optical monitoring of the intra-day variable blazar
S5 0716+71 with a dense temporal coverage over a total duration of 4 weeks
in February/March 1994. Four filters (BV Johnson and RI Cousins) were
used on a majority of the nights. The light curves of the blazar were derived
relative to two comparison stars present on the CCD frames. Intensity variations
of 0.05 mag from night-to-night were observed in half the cases and a
good correlation between the light curves in the different passbands was
noticed (as also for the observed intra-night variations). There seems to
be no correlation between flux and optical spectral index of the blazar.
In all, three prominent events of intra-night variability were detected,
each with a rate of
0.1 mag per hour, lasting for at least 3 hours.
Each of these flaring segments of the blazar light curves can be well
fitted with an exponential intensity profile whose rate of variation is
essentially the same for all the passbands. No clear event of ultra-rapid
fluctuations of the blazar on time scale
hour was detected in these
multi-colour data. Present observations have been carried out
during a low brightness level of the blazar and they have no large
amplitude variable events.
Key words: BL Lac objects: general -- BL Lac objects: individual: S5 0716+71 -- galaxies: photometry
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