V. N. Komarova
Russian Academy of Sciences
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Publication
Featured researches published by V. N. Komarova.
Astronomy and Astrophysics | 2001
A. J. Castro-Tirado; V. V. Sokolov; J. Gorosabel; J. M. Castro Cerón; J. Greiner; R.A.M.J. Wijers; B. L. Jensen; J. Hjorth; Sune Toft; H. Pedersen; E. Palazzi; E. Pian; N. Masetti; Ram Sagar; V. Mohan; A.K. Pandey; S.B. Pandey; S.N. Dodonov; T. A. Fatkhullin; V. L. Afanasiev; V. N. Komarova; A. V. Moiseev; R. Hudec; V. Simon; Paul M. Vreeswijk; E. Rol; Sylvio Klose; Bringfried Stecklum; Maria Rosa Zapatero-Osorio; Nicola Caon
Broad-band optical observations of the extraordi- narily bright optical afterglow of the intense gamma-ray burst GRB 991208 started � 2.1 days after the event and continued until 4 Apr 2000. The flux decay constant of the optical after- glow in the R-band is 2.30 ± 0.07 up to � 5 days, which
Astronomy and Astrophysics | 2004
Sergey Zharikov; Yu. A. Shibanov; R. E. Mennickent; V. N. Komarova; A. B. Koptsevich; G. Tovmassian
We report on deep UBVRI -imaging of the field of the 17.3 Myr radiopulsar PSR B0950+08 obtained with the ESO/VLT/FORS1. Firm detection of the candidate pulsar optical counterpart in the BVRI bands with the magnitudes
Astronomy and Astrophysics | 2008
S. V. Zharikov; Yu. A. Shibanov; D A Zyuzin; R. E. Mennickent; V. N. Komarova
B=27.06
Astronomy and Astrophysics | 2008
S. V. Zharikov; Yu. A. Shibanov; R. E. Mennickent; V. N. Komarova
± 0.35,
Astronomy and Astrophysics | 2004
J. M. Castro Cerón; J. Gorosabel; A. J. Castro-Tirado; V. V. Sokolov; V. L. Afanasiev; T. A. Fatkhullin; S. N. Dodonov; V. N. Komarova; Anatolii M. Cherepashchuk; K. A. Postnov; Ute Lisenfeld; J. Greiner; Sylvio Klose; J. Hjorth; Johan Peter Uldall Fynbo; H. Pedersen; E. Rol; Juergen Fliri; Markus Feldt; G. Feulner; Michael I. Andersen; B. L. Jensen; M. D. Pérez Ramírez; Frederick J. Vrba; Arne A. Henden; G. Israelian; Nial R. Tanvir
V=27.05
arXiv: Astrophysics | 2001
V. V. Sokolov; T. A. Fatkhullin; V. N. Komarova; E. R. Kasimova; V. I. Korchagin
± 0.15,
arXiv: Astrophysics | 2000
V. G. Kurt; V. N. Komarova; T. A. Fatkhullin; Vladimir V. Sokolov; A. B. Koptsevich; Yu. A. Shibanov
R_{\rm c}=26.49
Archive | 2010
A. S. Moskvitin; T. A. Fatkhullin; Vladimir V. Sokolov; V. N. Komarova
± 0.10 and
Archive | 2010
Andrew J. Drake; Stanislav G. Djorgovski; Ashish A. Mahabal; Matthew J. Graham; Roy Williams; T. A. Fatkhullin; V. N. Komarova; A. S. Moskvitin; Vladimir V. Sokolov; Tatiana N. Sokolova; Jose Luis Palacio Prieto; Marcio Catelan; E. Christensen; E. C. Beshore; S. M. Larson; R. H. McNaught; G. J. Garradd
I_{\rm c}=26.20
Archive | 2010
T. A. Fatkhullin; V. N. Komarova; A. S. Moskvitin; Vladimir V. Sokolov; Tatiana N. Sokolova; Andrew J. Drake; Stanislav G. Djorgovski; Ashish A. Mahabal; Matthew J. Graham; Roy Williams
± 0.17 enabled us to study, for the first time, the broadband spectrum of the object. The derived ~
