E
E. N. Sokov
Researcher at Russian Academy of Sciences
Publications - 17
Citations - 165
E. N. Sokov is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Exoplanet & Planet. The author has an hindex of 6, co-authored 13 publications receiving 144 citations.
Papers
More filters
Journal ArticleDOI
Benchmarking the power of amateur observatories for TTV exoplanets detection
Roman V. Baluev,Roman V. Baluev,E. N. Sokov,Vakhit Sh. Shaidulin,Vakhit Sh. Shaidulin,Iraida A. Sokova,Hugh R. A. Jones,Mikko Tuomi,Mikko Tuomi,Guillem Anglada-Escudé,Guillem Anglada-Escudé,P. Benni,C. Colazo,M. Schneiter,Carolina Villarreal D'Angelo,A. Burdanov,Eduardo Fernández-Lajús,Eduardo Fernández-Lajús,Özgür Baştürk,Veli-Pekka Hentunen,Stan Shadick +20 more
TL;DR: Baluev et al. as mentioned in this paper benchmarked the power of amateur observatories for TTV exoplanets detection using the Monthly Notices of the Royal Astronomical Society (MNRS).
Journal ArticleDOI
Kepler Object of Interest Network I. First results combining ground and space-based observations of Kepler systems with transit timing variations
C. von Essen,Aviv Ofir,S. Dreizler,Eric Agol,J. Freudenthal,Jonay I. González Hernández,Sven Wedemeyer,Vaishali Parkash,Hans J. Deeg,Sergio Hoyer,Brett M. Morris,A. C. Becker,L. Sun,Shenghong Gu,E. Herrero,Lev Tal-Or,Katja Poppenhaeger,Matthias Mallonn,Simon Albrecht,S. Khalafinejad,P. Boumis,C. Delgado-Correal,D. C. Fabrycky,Rimvydas Janulis,S. Lalitha,Alexios Liakos,Šarūnas Mikolaitis,M. L. Moyano D'Angelo,E. N. Sokov,E. Pakstiene,A. Popov,V. Krushinsky,Ignasi Ribas,S. Rusov,I. A. Sokova,G. Tautvaisiene,Xuan Wang +36 more
TL;DR: In this paper, the Kepler Object of Interest Network (KOINet) is proposed to complete the TTV curves of systems where Kepler did not cover the interaction timescales well.
Journal ArticleDOI
Kepler Object of Interest Network I. First results combining ground- and space-based observations of Kepler systems with transit timing variations
C. von Essen,Aviv Ofir,Aviv Ofir,Stefan Dreizler,Eric Agol,Eric Agol,Eric Agol,J. Freudenthal,Jesús Hernández,Sven Wedemeyer,Vaishali Parkash,Hans J. Deeg,Hans J. Deeg,Sergio Hoyer,Sergio Hoyer,Sergio Hoyer,Brett M. Morris,A. C. Becker,L. Sun,Shenghong Gu,E. Herrero,Lev Tal-Or,Lev Tal-Or,Katja Poppenhaeger,Matthias Mallonn,Simon Albrecht,S. Khalafinejad,P. Boumis,C. Delgado-Correal,D. C. Fabrycky,Rimvydas Janulis,S. Lalitha,Alexios Liakos,Šarūnas Mikolaitis,M. L. Moyano D'Angelo,E. N. Sokov,E. Pakštienė,A. A. Popov,V. Krushinsky,Ignasi Ribas,S. Rusov,Iraida A. Sokova,Gražina Tautvaišienė,Xuan Wang +43 more
TL;DR: The Kepler Object of Interest Network (KOINet) as discussed by the authors is a multi-site network formed of several telescopes located throughout America, Europe, and Asia to complete the TTV curves of systems where Kepler did not cover the interaction timescales well.
Journal ArticleDOI
The PHEMU15 catalogue and astrometric results of the Jupiter's Galilean satellite mutual occultation and eclipse observations made in 2014-2015
Eléonore Saquet,N. V. Emelyanov,V. Robert,V. Robert,Jean-Eudes Arlot,P. Anbazhagan,Kévin Baillié,J. Bardecker,Alexey A. Berezhnoy,M. Bretton,F. Campos,L. Capannoli,Benoit Carry,M. Castet,Y. Charbonnier,M. M. Chernikov,Apostolos A. Christou,François Colas,J.-F. Coliac,G. Dangl,O. Dechambre,M. Delcroix,A. Dias-Oliveira,C. Drillaud,Y. Duchemin,R. Dunford,P. Dupouy,C. K. Ellington,P. Fabre,V. A. Filippov,J. Finnegan,S. Foglia,D. Font,B. Gaillard,G. Galli,J. Garlitz,A. Gasmi,H. S. Gaspar,D. Gault,Kosmas Gazeas,T. George,S. Y. Gorda,D. L. Gorshanov,C. Gualdoni,K. Guhl,K. Halir,W. Hanna,X. Henry,D. Herald,G. Houdin,Y. Ito,I. S. Izmailov,J. Jacobsen,A. Jones,S. Kamoun,E. Kardasis,A. M. Karimov,M. Y. Khovritchev,A. M. Kulikova,J. Laborde,Valery Lainey,M. Lavayssière,P. Le Guen,A. Leroy,B. Loader,O. C. Lopez,A. Y. Lyashenko,P. G. Lyssenko,D. I. Machado,N. Maigurova,J. Manek,Andrea Marchini,T. Midavaine,J. Montier,B. E. Morgado,K. N. Naumov,A. Nedelcu,Jeffrey A. Newman,J. M. Ohlert,Arto Oksanen,H. Pavlov,E. Petrescu,A. Pomazan,Marcel Popescu,A. Pratt,V. N. Raskhozhev,J. M. Resch,D. Robilliard,E. Roschina,E. Rothenberg,M. Rottenborn,S. Rusov,F. Saby,L. F. Saya,G. Selvakumar,F. Signoret,Viacheslav Slesarenko,E. N. Sokov,J. Soldateschi,A. Sonka,G. Soulie,John Talbot,V. G. Tejfel,William Thuillot,Brad Timerson,R. Toma,S. Torsellini,L. L. Trabuco,P. Traverse,V. Tsamis,M. Unwin,F. Van Den Abbeel,H. Vandenbruaene,R. Vasundhara,Yu. I. Velikodsky,Alain Vienne,J. Vilar,J. M. Vugnon,N. Wuensche,P. Zeleny +119 more
TL;DR: In this paper, the authors focused on processing the complete photometric observations data base to compute new accurate astrometric positions from the light curves of the mutual occultations and eclipses.
Journal ArticleDOI
First results of the Kourovka Planet Search: discovery of transiting exoplanet candidates in the first three target fields
A. Burdanov,P. Benni,V. Krushinsky,A. A. Popov,E. N. Sokov,Iraida A. Sokova,S. Rusov,Artem Yu. Lyashenko,Kirill Ivanov,Alexei Moiseev,D. A. Rastegaev,V. V. Dyachenko,Y. Y. Balega,Özgür Baştürk,I. Özavcı,Damian Puchalski,Alessandro Marchini,Ramon Naves,Stan Shadick,M. Bretton +19 more
Abstract: We present the first results of our search for transiting exoplanet candidates as part of the Kourovka Planet Search (KPS) project. The primary objective of the project is to search for new hot Jupiters which transit their host stars, mainly in the Galactic plane, in the $R_c$ magnitude range of 11 to 14 mag. Our observations were performed with the telescope of the MASTER robotic network, installed at the Kourovka astronomical observatory of the Ural Federal University (Russia), and the Rowe-Ackermann Schmidt Astrograph, installed at the private Acton Sky Portal Observatory (USA). As test observations, we observed three celestial fields of size $2\times2$ deg$^2$ during the period from 2012 to 2015. As a result, we discovered four transiting exoplanet candidates among the 39000 stars of the input catalogue. In this paper, we provide the description of the project and analyse additional photometric, spectral, and speckle interferometric observations of the discovered transiting exoplanet candidates. Three of the four transiting exoplanet candidates are most likely astrophysical false positives, while the nature of the fourth (most promising) candidate remains to be ascertained. Also, we propose an alternative observing strategy that could increase the project's exoplanet haul.