<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Zola, S.</style></author><author><style face="normal" font="default" size="100%">Valtonen, M.</style></author><author><style face="normal" font="default" size="100%">Ciprini, S.</style></author><author><style face="normal" font="default" size="100%">Reichart, D. E.</style></author><author><style face="normal" font="default" size="100%">Moore, J. P.</style></author><author><style face="normal" font="default" size="100%">LaCluyze, A. P.</style></author><author><style face="normal" font="default" size="100%">Ivarsen, K. M.</style></author><author><style face="normal" font="default" size="100%">Groom, R.</style></author><author><style face="normal" font="default" size="100%">Stranger, K.</style></author><author><style face="normal" font="default" size="100%">Sadakane, K.</style></author><author><style face="normal" font="default" size="100%">Matsumoto, K.</style></author><author><style face="normal" font="default" size="100%">Kagitani, M.</style></author><author><style face="normal" font="default" size="100%">Okano, S.</style></author><author><style face="normal" font="default" size="100%">Sakanoi, T.</style></author><author><style face="normal" font="default" size="100%">Provencal, J.</style></author><author><style face="normal" font="default" size="100%">Dalessio, J.</style></author><author><style face="normal" font="default" size="100%">Drozdz, M.</style></author><author><style face="normal" font="default" size="100%">Siwak, M.</style></author><author><style face="normal" font="default" size="100%">Gazeas, K.</style></author><author><style face="normal" font="default" size="100%">Ramazani, V. Fallah</style></author><author><style face="normal" font="default" size="100%">Kidger, M.</style></author><author><style face="normal" font="default" size="100%">Naves, R.</style></author><author><style face="normal" font="default" size="100%">Campas, Montse</style></author><author><style face="normal" font="default" size="100%">Jermak, H.</style></author><author><style face="normal" font="default" size="100%">Steele, I. A.</style></author><author><style face="normal" font="default" size="100%">Sonbas, E.</style></author><author><style face="normal" font="default" size="100%">Er, H.</style></author><author><style face="normal" font="default" size="100%">Zejmo, M.</style></author><author><style face="normal" font="default" size="100%">Caton, D. B.</style></author><author><style face="normal" font="default" size="100%">Poyner, G.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">A strong optical activity of the OJ287 blazar</style></title><short-title><style face="normal" font="default" size="100%">The Astronomer's Telegram</style></short-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">AGN</style></keyword><keyword><style  face="normal" font="default" size="100%">Black Hole</style></keyword><keyword><style  face="normal" font="default" size="100%">Blazar</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2016</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2016/03/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2016ATel.8768....1Z</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">8768</style></volume><pages><style face="normal" font="default" size="100%">1</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">We have continued monitoring the blazar OJ287 in the optical at several sites after its November/December, 2015 outburst. After a further large outburst that started in the beginning of February, 2016 (Atels #8667, #8697, #8705) OJ287 remained brighter than 14th magnitude [in R] for the rest of the month.</style></abstract></record></records></xml>