Bibcode
Heidt, J.; Peila, A.; Chiaberge, M.; Lanteri, L.; de Francesco, G.; Villata, M.; Raiteri, C. M.; Ghisellini, G.; Tosti, G.; Fiorucci, M.; Shakhovskoy, N.; Efimov, Yu. S.; Honeycut, R. K.; Robertson, J. W.; Turner, G. W.; Boltwood, P.; Kidger, M. R.; Rekola, R.; Hanski, M.; Pietila, H.; Katajainen, S.; Heinamaki, P.; Nilsson, K.; Pursimo, T.; Takalo, L. O.; Sillanpaa, A.
Bibliographical reference
Astronomy and Astrophysics, v.315, p.L13-L16
Advertised on:
11
1996
Journal
Citations
112
Refereed citations
94
Description
An international monitoring project, called OJ-94, was set up with the
aim of monitoring blazar OJ 287 during the predicted optical outburst
(in fall 1994, Sillanpaa et al. 1988ApJ...325..628S) and the predicted
secondary outburst (in winter 1995-1996, Sillanpaa et al.
1996A&A...305L..17S). The most prominent features in the OJ 287
light curve during the period covered by the project are the large
outburst in September-December 1994, reaching the maximum at the
beginning of November, and the secondary outburst peaking just at
Christmas 1995. Both these outbursts occurred almost exactly at the
predicted times.