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Browsing Научные публикации в Scopus by Author "Oksanen A."

Browsing Научные публикации в Scopus by Author "Oksanen A."

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  • Eclipses during the 2010 eruption of the recurrent nova U Scorpii 
    Schaefer B.; Pagnotta A.; Lacluyze A.; Reichart D.; Ivarsen K.; Haislip J.; Nysewander M.; Moore J.; Oksanen A.; Worters H.; Sefako R.; Mentz J.; Dvorak S.; Gomez T.; Harris B.; Henden A.; Tan T.; Templeton M.; Allen W.; Monard B.; Rea R.; Roberts G.; Stein W.; Maehara H.; Richards T.; Stockdale C.; Krajci T.; Sjoberg G.; McCormick J.; Revnivtsev M.; Molkov S.; Suleimanov V.; Darnley M.; Bode M.; Handler G.; Lepine S.; Shara M. (2011)
    The eruption of the recurrent nova U Scorpii on 2010 January 28 is now the all-time best observed nova event. We report 36,776 magnitudes throughout its 67 day eruption, for an average of one measure every 2.6 minutes. ...
  • Superoutburst of CR Bootis: Estimation of mass ratio of a typical AMCVn star by stage A superhumps 
    Isogai K.; Kato T.; Ohshima T.; Kasai K.; Oksanen A.; Masumoto K.; Fukushima D.; Maeda K.; Kawabata M.; Matsuda R.; Kojiguchi N.; Sugiura Y.; Takeda N.; Matsumoto K.; Itoh H.; Pavlenko E.; Antonyuk K.; Antonyuk O.; Pit N.; Sosnovskij A.; Baklanov A.; Babina J.; Sklyanov A.; Kiyota S.; Hambsch F.; Littlefield C.; Maeda Y.; Cook L.; Masi G.; Dubovsky P.; Novák R.; Dvorak S.; Imada A.; Nogami D. (2016)
    © The Author 2016.We report on two superoutbursts of the AMCVn-type object CR Boo in 2014 April-March and 2015 May-June. A precursor outburst accompanied both of these superoutbursts. During the rising branch of the main ...
  • Survey of period variations of superhumps in SU UMa-type dwarf novae. VI. The sixth year (2013-2014) 
    Kato T.; Dubovsky P.; Kudzej I.; Hambsch F.; Miller I.; Ohshima T.; Nakata C.; Kawabata M.; Nishino H.; Masumoto K.; Mizoguchi S.; Yamanaka M.; Matsumoto K.; Sakai D.; Fukushima D.; Matsuura M.; Bouno G.; Takenaka M.; Nakagawa S.; Noguchi R.; Iino E.; Pickard R.; Maeda Y.; Henden A.; Kasai K.; Kiyota S.; Akazawa H.; Imamura K.; De Miguel E.; Maehara H.; Monard B.; Pavlenko E.; Antonyuk K.; Pit N.; Antonyuk O.; Baklanov A.; Ruiz J.; Richmond M.; Oksanen A.; Harlingten C.; Shugarov S.; Chochol D.; Masi G.; Nocentini F.; Schmeer P.; Bolt G.; Nelson P.; Ulowetz J.; Sabo R.; Goff W.; Stein W.; Michel R.; Dvorak S.; Voloshina I.; Metlov V.; Katysheva N.; Neustroev V.; Sjoberg G.; Littlefield C.; Dębski B.; Sowicka P.; Klimaszewski M.; Curyło M.; Morelle E.; Curtis I.; Iwamatsu H.; Butterworth N.; Andreev M.; Parakhin N.; Sklyanov A.; Shiokawa K.; Novák R.; Irsmambetova T.; Itoh H.; Ito Y.; Hirosawa K.; Denisenko D.; Kochanek C.; Shappee B.; Stanek K.; Prieto J.; Itagaki K.; Stubbings R. (2014)
    © The Author 2014. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved. Continuing the project undertaken by Kato et al. (2009), we collected times of superhump maxima ...
  • Survey of period variations of superhumps in SU UMa-type dwarf novae. VII. the seventh year (2014-2015) 
    Kato T.; Hambsch F.; Dubovsky P.; Kudzej I.; Monard B.; Miller I.; Itoh H.; Kiyota S.; Masumoto K.; Fukushima D.; Kinoshita H.; Maeda K.; Mikami J.; Matsuda R.; Kojiguchi N.; Kawabata M.; Takenaka M.; Matsumoto K.; De Miguel E.; Maeda Y.; Ohshima T.; Isogai K.; Pickard R.; Henden A.; Kafka S.; Akazawa H.; Otani N.; Ishibashi S.; Ogi M.; Tanabe K.; Imamura K.; Stein W.; Kasai K.; Vanmunster T.; Starr P.; Oksanen A.; Pavlenko E.; Antonyuk O.; Antonyuk K.; Sosnovskij A.; Pit N.; Babina J.; Sklyanov A.; Novák R.; Dvorak S.; Michel R.; Masi G.; Littlefield C.; Ulowetz J.; Shugarov S.; Golysheva P.; Chochol D.; Krushevska V.; Ruiz J.; Tordai T.; Morelle E.; Sabo R.; Maehara H.; Richmond M.; Katysheva N.; Hirosawa K.; Goff W.; Dubois F.; Logie L.; Rau S.; Voloshina I.; Andreev M.; Shiokawa K.; Neustroev V.; Sjoberg G.; Zharikov S.; James N.; Bolt G.; Crawford T.; Buczynski D.; Cook L.; Kochanek C.; Shappee B.; Stanek K.; Prieto J.; Denisenko D.; Nishimura H.; Mukai M.; Kaneko S.; Ueda S.; Stubbings R.; Moriyama M.; Schmeer P.; Muyllaert E. (2015)
    © The Author 2015. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved. Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of ...
  • Survey of period variations of superhumps in SU UMa-type dwarf novae. VIII. The eighth year (2015-2016) 
    Kato T.; Hambsch F.; Monard B.; Vanmunster T.; Maeda Y.; Miller I.; Itoh H.; Kiyota S.; Isogai K.; Kimura M.; Imada A.; Tordai T.; Akazawa H.; Tanabe K.; Otani N.; Ogi M.; Ando K.; Takigawa N.; Dubovsky P.; Kudzej I.; Shugarov S.; Katysheva N.; Golysheva P.; Gladilina N.; Chochol D.; Starr P.; Kasai K.; Pickard R.; De Miguel E.; Kojiguchi N.; Sugiura Y.; Fukushima D.; Yamada E.; Uto Y.; Kamibetsunawa T.; Tatsumi T.; Takeda N.; Matsumoto K.; Cook L.; Pavlenko E.; Babina J.; Pit N.; Antonyuk O.; Antonyuk K.; Sosnovskij A.; Baklanov A.; Kafka S.; Stein W.; Voloshina I.; Ruiz J.; Sabo R.; Dvorak S.; Stone G.; Andreev M.; Antipin S.; Zubareva A.; Zaostrojnykh A.; Richmond M.; Shears J.; Dubois F.; Logie L.; Rau S.; Vanaverbeke S.; Simon A.; Oksanen A.; Goff W.; Bolt G.; Ebski B.; Kochanek C.; Shappee B.; Stanek K.; Prieto J.; Stubbings R.; Muyllaert E.; Hiraga M.; Horie T.; Schmeer P.; Hirosawa K. (2016)
    © The Author 2016.Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for 128 SUUMa-type dwarf novae observed mainly during the 2015-2016 season and characterized ...
  • The 72-h WEBT microvariability observation of blazar S5 0716 + 714 in 2009 
    Bhatta G.; Webb J.; Hollingsworth H.; Dhalla S.; Khanuja A.; Bachev R.; Blinov D.; Bottcher M.; Bravo Calle O.; Calcidese P.; Capezzali D.; Carosati D.; Chigladze R.; Collins A.; Coloma J.; Efimov Y.; Gupta A.; Hu S.; Kurtanidze O.; Lamerato A.; Larionov V.; Lee C.; Lindfors E.; Murphy B.; Nilsson K.; Ohlert J.; Oksanen A.; Pääkkönen P.; Pollock J.; Rani B.; Reinthal R.; Rodriguez D.; Ros J.; Roustazadeh P.; Sagar R.; Sanchez A.; Shastri P.; Sillanpää A.; Strigachev A.; Takalo L.; Vennes S.; Villata M.; Villforth C.; Wu J.; Zhou X. (2013)
    Context. The international Whole Earth Blazar Telescope (WEBT) consortium planned and carried out three days of intensive micro-variability observations of S5 0716 + 714 from February 22, 2009 to February 25, 2009. This ...

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