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Are there transit timing variations for the exoplanet qatar-1b?

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dc.contributor.author Su, Li-Hsin
dc.contributor.author Jiang, Ing-Guey
dc.contributor.author Sariya, Devesh P
dc.contributor.author Lee, Chiao-Yu
dc.contributor.author Yeh, Li-Chin
dc.contributor.author Mannaday, Vineet Kumar
dc.contributor.author Thaku, Parijat
dc.contributor.author Chand, Swadesh
dc.contributor.author Shlyapnikov, A. A
dc.contributor.author Moskvin, V. V
dc.contributor.author Ignatov, Vladimir
dc.contributor.author Mkrtichian, David
dc.contributor.author Griv, Evgeny
dc.contributor.author Sahu, D. K
dc.date.accessioned 2021-06-25T12:47:43Z
dc.date.available 2021-06-25T12:47:43Z
dc.date.issued 2021-03-01
dc.identifier.citation The Astronomical Journal, Vol. 161, No. 3, 108 en_US
dc.identifier.issn 1538-4357
dc.identifier.uri http://hdl.handle.net/2248/7692
dc.description Restricted Access en_US
dc.description.abstract Motivated by the unsettled conclusion on whether there are any transit timing variations (TTVs) for the exoplanet Qatar-1b, 10 new transit light curves are presented and a TTV analysis with a baseline of 1400 epochs is performed. Because the linear model provides a good fit with a reduced chi-square of x2red=2.59 and the false-alarm probabilities of the possible TTV frequencies are as large as 35%, our results are consistent with a null-TTV model. Nevertheless, a new ephemeris with a reference time of T0 = 2455647.63360 ± 0.00008 (BJD) and a period of P = 1.4200236 ± 0.0000001 (day) is obtained. In addition, the updated orbital semimajor axis and planetary radius in units of stellar radius are provided, and the lower limit of the modified stellar tidal quality factor is also determined. en_US
dc.language.iso en en_US
dc.publisher IOP Publishing en_US
dc.relation.uri https://doi.org/10.3847/1538-3881/abd4d8
dc.rights © The American Astronomical Society
dc.subject Exoplanet astronomy en_US
dc.subject Transit photometry en_US
dc.title Are there transit timing variations for the exoplanet qatar-1b? en_US
dc.type Article en_US


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