VRI bands CCD photometric observations of the BL Lac object OJ 287 have been carried out during the period from October, 1994 to May, 1996. OJ 287 underwent two major outbursts during our observations. The first peak (V 14.0 mag.) occurred in the first half of November, 1994 and faded out to 16.5 mag within 150 days. The second peak (14.0 mag.) was observed in late December, 1995. The latter peak continued at nearly the same brightness until May, 1996. Such a long lasting outburst has never been reported for OJ 287. Color indices (V -- R and V --I) remained nearly constant during the outbursts. Key Words : BL Lac objects -- CCD Photometry -- OJ287 I. INTRODUCTION The BL Lac object OJ 287 has attracted attentions of many astronomers worki...
Abstract. Results of BV RI CCD photometric monitor-ing and fast photometry in the I band for the bla...
Two guest‐observer XMM‐Newton observations of the peculiar blazar OJ 287 in 2005 are briefly present...
The proper understanding of blazar variability at the various electromagnetic spectral bands is one ...
VRI-band CCD photometric observations of the BL Lac object OJ 287 have been carried out from 1995 Fe...
© 2016 The Authors.We present recent optical photometric observations of the blazar OJ 287 taken dur...
We present intensive optical, infrared, and radio monitoring observations of the BL Lac object OJ ...
We present long-term optical multi-band photometric monitoring of the blazar OJ 287 from 6 March 201...
We present the results of our optical monitoring of the BL Lacertae object OJ 287 during the first h...
Results of BVRI CCD photometric monitoring and fast photometry in the I band for the blazar OJ 287 ...
Context. The blazar OJ 287 has been proposed as binary black hole system based on its periodic optic...
The results of optical photometric $(BVRI)$ monitoring of three BL Lac objects over a time interval ...
In early 1983, OJ 287 was seen to undergo an outburst in its optical and infrared emission. The auth...
OJ 287 is a BL Lac object at redshift z = 0.306 that has shown double-peaked bursts at regular inter...
The paper presents the first evidence for the long-term near-infrared brightness, colour and spectra...
We report on historical optical outbursts in the OJ287 system in 1900 and 1913, detected o...
Abstract. Results of BV RI CCD photometric monitor-ing and fast photometry in the I band for the bla...
Two guest‐observer XMM‐Newton observations of the peculiar blazar OJ 287 in 2005 are briefly present...
The proper understanding of blazar variability at the various electromagnetic spectral bands is one ...
VRI-band CCD photometric observations of the BL Lac object OJ 287 have been carried out from 1995 Fe...
© 2016 The Authors.We present recent optical photometric observations of the blazar OJ 287 taken dur...
We present intensive optical, infrared, and radio monitoring observations of the BL Lac object OJ ...
We present long-term optical multi-band photometric monitoring of the blazar OJ 287 from 6 March 201...
We present the results of our optical monitoring of the BL Lacertae object OJ 287 during the first h...
Results of BVRI CCD photometric monitoring and fast photometry in the I band for the blazar OJ 287 ...
Context. The blazar OJ 287 has been proposed as binary black hole system based on its periodic optic...
The results of optical photometric $(BVRI)$ monitoring of three BL Lac objects over a time interval ...
In early 1983, OJ 287 was seen to undergo an outburst in its optical and infrared emission. The auth...
OJ 287 is a BL Lac object at redshift z = 0.306 that has shown double-peaked bursts at regular inter...
The paper presents the first evidence for the long-term near-infrared brightness, colour and spectra...
We report on historical optical outbursts in the OJ287 system in 1900 and 1913, detected o...
Abstract. Results of BV RI CCD photometric monitor-ing and fast photometry in the I band for the bla...
Two guest‐observer XMM‐Newton observations of the peculiar blazar OJ 287 in 2005 are briefly present...
The proper understanding of blazar variability at the various electromagnetic spectral bands is one ...