Электронный архив

Просмотр по автору "Godunova V."

Просмотр по автору "Godunova V."

Отсортировать по:Сортировать:Результаты поиска на странице:

  • Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using Its General Relativity Centenary Flare: Improved Orbital Parameters 
    Dey L.; Valtonen M.; Gopakumar A.; Zola S.; Hudec R.; Pihajoki P.; Ciprini S.; Matsumoto K.; Sadakane K.; Kidger M.; Nilsson K.; Mikkola S.; Sillanpää A.; Takalo L.; Lehto H.; Berdyugin A.; Piirola V.; Jermak H.; Baliyan K.; Pursimo T.; Caton D.; Alicavus F.; Baransky A.; Blay P.; Boumis P.; Boyd D.; Torrent M.; Campos F.; Gómez J.; Chandra S.; Chavushyan V.; Dalessio J.; Debski B.; Drozdz M.; Er H.; Erdem A.; Pérez A.; Ramazani V.; Filippenko A.; Gafton E.; Ganesh S.; Garcia F.; Gazeas K.; Godunova V.; Pinilla F.; Gopinathan M.; Haislip J.; Harmanen J.; Hurst G.; Janík J.; Jelinek M.; Joshi A.; Kagitani M.; Karjalainen R.; Kaur N.; Keel W.; Kouprianov V.; Kundera T.; Kurowski S.; Kvammen A.; Lacluyze A.; Lee B.; Liakos A.; Lindfors E.; De Haro J.; Mugrauer M.; Nogues R.; Neely A.; Nelson R.; Ogloza W.; Okano S.; Pajdosz-Śmierciak U.; Pandey J.; Perri M.; Poyner G.; Provencal J.; Raj A.; Reichart D.; Reinthal R.; Reynolds T.; Saario J.; Sadegi S.; Sakanoi T.; González J.; Sameer; Schweyer T.; Simon A. (2018)
    © 2018. The American Astronomical Society. All rights reserved. Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational ...
  • Discovery of standstills in the SU UMa-type dwarf nova NY Serpentis 
    Kato T.; Pavlenko E.; Pit N.; Antonyuk K.; Antonyuk O.; Babina J.; Baklanov A.; Sosnovskij A.; Belan S.; Maeda Y.; Sugiura Y.; Sumiya S.; Matsumoto H.; Ito D.; Nikai K.; Kojiguchi N.; Matsumoto K.; Dubovsky P.; Kudzej I.; Medulka T.; Wakamatsu Y.; Ohnishi R.; Seki T.; Isogai K.; Simon A.; Romanjuk Y.; Baransky A.; Sergeev A.; Godunova V.; Izviekova I.; Kozlov V.; Sklyanov A.; Zhuchkov R.; Gutaev A.; Ponomarenko V.; Vasylenko V.; Miller I.; Kasai K.; Dvorak S.; Menzies K.; De Miguel E.; Brincat S.; Pickard R. (2019)
    © The Author(s) 2019. We found that the SU UMa-type dwarf nova NY Ser in the period gap [orbital period 0.097558(6) d] showed standstills twice in 2018. This is the first clear demonstration of a standstill occurring between ...
  • Long-period SUUMa dwarf nova V1006 Cygni: Outburst activity and variability at different brightness states in 2015 - 2017 
    Godunova V.; Sokolov I.; Rudakov I. (2018)
    © 2018, Astronomical Institute, Slovak Academy of Sciences. CCD photometric observations of the dwarf nova V1006 Cyg were carried out in 2015 { 2017 with 11 telescopes located at 7 observatories. They covered the 2015 ...
  • MASTER OT J172758.09+380021.5: a peculiar ER UMa-type dwarf nova, probably a missed nova in the recent past 
    Pavlenko E.; Kato T.; Antonyuk K.; Pit N.; Keir L.; Udovichenko S.; Dubovský P.; Sosnovskij A.; Antonyuk O.; Shimansky V.; Gabdeev M.; Rakhmatullaeva F.; Kokhirova G.; Belan S.; Simon A.; Baklanov A.; Kojiguchi N.; Godunova V. (2021)
    A CCD photometry of the dwarf nova MASTER OT J172758.09 +380021.5 was carried out in 2019 during 134 nights. Observations covered three superoutbursts, five normal outbursts and quiescence between them. The available ASASSN ...
  • Polarization and spectral energy distribution in OJ 287 during the 2016/17 outbursts 
    Valtonen M.; Zola S.; Jermak H.; Ciprini S.; Hudec R.; Dey L.; Gopakumar A.; Reichart D.; Caton D.; Gazeas K.; Matsumoto K.; Ogloza W.; Drozdz M.; Alicavus F.; Baransky O.; Berdyugin A.; Boumis P.; Bufan Y.; Debski B.; Er H.; Erdem A.; Godunova V.; Haque S.; Hoette V.; Janik J.; Kidger M.; Kundera T.; Kurowski S.; Liakos A.; Mohammed I.; Nilsson K.; Pajdosz U.; Piirola V.; Pursimo T.; Rajkumar B.; Simon A.; Siwak M.; Sonbas E.; Steele I.; Vasylenko V.; Zejmo M.; Zielinski P. (2017)
    © 2017 by the authors. We report optical photometric and polarimetric observations of the blazar OJ 287 gathered during 2016/17. The high level of activity, noticed after the General Relativity Centenary flare, is argued ...
  • Spitzer Observations of the Predicted Eddington Flare from Blazar OJ 287 
    Laine S.; Dey L.; Valtonen M.; Gopakumar A.; Zola S.; Komossa S.; Kidger M.; Pihajoki P.; Gómez J.L.; Caton D.; Ciprini S.; Drozdz M.; Gazeas K.; Godunova V.; Haque S.; Hildebrandt F.; Hudec R.; Jermak H.; Kong A.K.H.; Lehto H.; Liakos A.; Matsumoto K.; Mugrauer M.; Pursimo T.; Reichart D.E.; Simon A.; Siwak M.; Sonbas E. (2020)
    © 2020. The American Astronomical Society. All rights reserved.. Binary black hole (BH) central engine description for the unique blazar OJ 287 predicted that the next secondary BH impact-induced bremsstrahlung flare should ...
  • Stochastic Modeling of Multiwavelength Variability of the Classical BL Lac Object OJ 287 on Timescales Ranging from Decades to Hours 
    Goyal A.; Stawarz; Zola S.; Marchenko V.; Soida M.; Nilsson K.; Ciprini S.; Baran A.; Ostrowski M.; Wiita P.; Gopal-Krishna; Siemiginowska A.; Sobolewska M.; Jorstad S.; Marscher A.; Aller M.; Aller H.; Hovatta T.; Caton D.; Reichart D.; Matsumoto K.; Sadakane K.; Gazeas K.; Kidger M.; Piirola V.; Jermak H.; Alicavus F.; Baliyan K.; Baransky A.; Berdyugin A.; Blay P.; Boumis P.; Boyd D.; Bufan Y.; Torrent M.; Campos F.; Gómez J.; Dalessio J.; Debski B.; Dimitrov D.; Drozdz M.; Er H.; Erdem A.; Pérez A.; Ramazani V.; Filippenko A.; Gafton E.; Garcia F.; Godunova V.; Pinilla F.; Gopinathan M.; Haislip J.; Haque S.; Harmanen J.; Hudec R.; Hurst G.; Ivarsen K.; Joshi A.; Kagitani M.; Karaman N.; Karjalainen R.; Kaur N.; Kozieł-Wierzbowska D.; Kuligowska E.; Kundera T.; Kurowski S.; Kvammen A.; Lacluyze A.; Lee B.; Liakos A.; Haro J.; Moore J.; Mugrauer M.; Nogues R.; Neely A.; Ogloza W.; Okano S.; Pajdosz U.; Pandey J.; Perri M.; Poyner G.; Provencal J.; Pursimo T.; Raj A.; Rajkumar B.; Reinthal R.; Reynolds T.; Saario J.; Sadegi S. (2018)
    © 2018. The American Astronomical Society. All rights reserved.. We present the results of our power spectral density analysis for the BL Lac object OJ 287, utilizing the Fermi-LAT survey at high-energy γ-rays, Swift-XRT ...
  • The astrometric Gaia-FUN-SSO observation campaign of 99942 Apophis 
    Thuillot W.; Bancelin D.; Ivantsov A.; Desmars J.; Assafin M.; Eggl S.; Hestroffer D.; Rocher P.; Carry B.; David P.; Abe L.; Andreev M.; Arlot J.; Asami A.; Ayvasian V.; Baransky A.; Belcheva M.; Bendjoya P.; Bikmaev I.; Burkhonov O.; Camci U.; Carbognani A.; Colas F.; Devyatkin A.; Ehgamberdiev S.; Enikova P.; Eyer L.; Galeev A.; Gerlach E.; Godunova V.; Golubaev A.; Gorshanov D.; Gumerov R.; Hashimoto N.; Helvaci M.; Ibryamov S.; Inasaridze R.; Khamitov I.; Kostov A.; Kozhukhov A.; Kozyryev Y.; Krugly Y.; Kryuchkovskiy V.; Kulichenko N.; Maigurova N.; Manilla-Robles A.; Martyusheva A.; Molotov I.; Nikolov G.; Nikolov P.; Nishiyama K.; Okumura S.; Palaversa L.; Parmonov O.; Peng Q.; Petrova S.; Pinigin G.; Pomazan A.; Rivet J.; Sakamoto T.; Sakhibullin N.; Sergeev O.; Sergeyev A.; Shulga O.; Suarez O.; Sybiryakova Y.; Takahashi N.; Tarady V.; Todd M.; Urakawa S.; Uysal O.; Vaduvescu O.; Vovk V.; Zhang X. (2015)
    © 2015 ESO. Aims. Astrometric observations performed by the Gaia Follow-Up Network for Solar System Objects (Gaia-FUN-SSO) play a key role in ensuring that moving objects first detected by ESA's Gaia mission remain recoverable ...

Поиск в электронном архиве

Просмотр

Моя учетная запись