First detection of exoplanet transits with the SAO RAS 1-m telescope

dc.contributor.author	Valyavin G.
dc.contributor.author	Valeev A.
dc.contributor.author	Gadelshin D.
dc.contributor.author	Moskvitin A.
dc.contributor.author	Grauzhanina A.
dc.contributor.author	Galazutdinov G.
dc.date.accessioned	2018-09-18T20:31:01Z
dc.date.available	2018-09-18T20:31:01Z
dc.date.issued	2015
dc.identifier.issn	1990-3413
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/140686
dc.description.abstract	© Pleiades Publishing, Ltd., 2015. We present the results of observations of single exoplanet transits conducted with the SAO RAS 1-m telescope. We studied two exoplanets with different eclipse depths: WASP-43b and WASP-104b. Both transits were detected with different degrees of accuracy depending on the eclipse depth and observing conditions. The typical accuracy of registration of the transit amplitude in the broadband V filter of the Johnson system is (formula presented). We also present the characteristic time moments of the transits. Based on the obtained results, a further program of exoplanet research at SAO RAS has been developed.
dc.relation.ispartofseries	Astrophysical Bulletin
dc.subject	Planetary systems
dc.title	First detection of exoplanet transits with the SAO RAS 1-m telescope
dc.type	Article
dc.relation.ispartofseries-issue	3
dc.relation.ispartofseries-volume	70
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	315
dc.source.id	SCOPUS19903413-2015-70-3-SID84943414935

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.