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dc.contributor.authorPetrucci, R.
dc.contributor.authorMancini, L.
dc.contributor.authorSouthworth, J.
dc.contributor.authorCiceri, S.
dc.contributor.authorD'Ago, G.
dc.contributor.authorBruni, I.
dc.contributor.authorRaetz, St
dc.contributor.authorNowak, G.
dc.contributor.authorOhlert, J.
dc.contributor.authorPuchalski, D.
dc.contributor.authorSaral, G.
dc.contributor.authorDerman, E.
dc.contributor.authorHenning, T.
dc.contributor.authorSeeliger, M.
dc.contributor.authorJofre, E.
dc.contributor.authorMaciejewski, G.
dc.contributor.authorDimitrov, D.
dc.date.accessioned2021-03-05T08:06:05Z
dc.date.available2021-03-05T08:06:05Z
dc.date.issued2016
dc.identifier.citationMaciejewski G., Dimitrov D., Mancini L., Southworth J., Ciceri S., D'Ago G., Bruni I., Raetz S., Nowak G., Ohlert J., et al., "New Transit Observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b and WASP-39 b", ACTA ASTRONOMICA, cilt.66, ss.55-74, 2016
dc.identifier.issn0001-5237
dc.identifier.otherav_9726df59-87b0-4f5c-a1f2-c50b9571074e
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/101750
dc.description.abstractWe present new transit light curves for planets in six extrasolar planetary systems. They were acquired with 0.4-2.2 m telescopes located in west Asia, Europe, and South America. When combined with literature data, they allowed us to redetermine system parameters in a homogeneous way. Our results for individual systems are in agreement with values reported in previous studies. We refined transit ephemerides and reduced uncertainties of orbital periods by a factor between 2 and 7. No sign of any variations in transit times was detected for the planets studied.
dc.language.isoeng
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.titleNew Transit Observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b and WASP-39 b
dc.typeMakale
dc.relation.journalACTA ASTRONOMICA
dc.contributor.departmentNicolaus Copernicus University , ,
dc.identifier.volume66
dc.identifier.issue1
dc.identifier.startpage55
dc.identifier.endpage74
dc.contributor.firstauthorID229403


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