Revisiting KELT-19Ab, WASP-156b, and WASP-121b in the TESS Era
نویسندگان
چکیده
Abstract We present a re-analysis of transit depths KELT-19Ab, WASP-156b, and WASP-121b, including data from the Transiting Exoplanet Survey Satellite (TESS). The large ?21? TESS pixels point-spread function result in significant contamination stellar flux by nearby objects. use Gaia to fit for remove this contribution, providing general-purpose software correction. find all three sources have larger inclination, compared earlier work. For we significantly smaller values (13.°5) inclination when using 30 minute cadence 2 data. Using simulations, demonstrate that radius ratio exoplanet star ( R p / * ) is biased small relative taken with sampling interval although oversampling corrections mitigate bias. This particularly important deriving subpercent differences between bands. band 7.5 ? than previous work but consistent within ?2 WASP-156b WASP-121b. difference could be due specific choices analysis, not necessarily presence atmospheric features. KELT-19Ab possibly favors haze-dominated atmosphere. do evidence ?0.95 ? m water feature contaminating these stars show photometric precision 500 ppm about 200 observations across entire transit, detectable more narrow z -band.
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ژورنال
عنوان ژورنال: The Astronomical Journal
سال: 2022
ISSN: ['1538-3881', '0004-6256']
DOI: https://doi.org/10.3847/1538-3881/ac3b4e