Precovery of Transiting Exoplanet Survey Satellite Single Transits with Kilodegree Extremely Little Telescope

During the Transiting Exoplanet Survey Satellite (TESS) prime mission, 74% of the sky area will have an observational baseline of only 27 days. For planets with orbital periods longer than 13.5 days, TESS can capture only one or two transits, and the planet ephemerides will be difficult to determine...

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Veröffentlicht in:	The Astronomical journal 2019-01, Vol.157 (1), p.37
Hauptverfasser:	Yao, Xinyu, Pepper, Joshua, Scott Gaudi, B., Labadie-Bartz, Jonathan, Beatty, Thomas G., Colón, Knicole D., James, David J., Kuhn, Rudolf B., Lund, Michael B., Rodriguez, Joseph E., Siverd, Robert J., Stassun, Keivan G., Stevens, Daniel J., Villanueva, Steven, Bayliss, Daniel
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Ephemerides Extrasolar planets Gas giant planets Hubble Space Telescope James Webb Space Telescope Jupiter Light curve methods: data analysis Orbits Photometry Planet detection Planet ephemerides planets and satellites: detection planets and satellites: general Satellites Sky surveys (astronomy) Space telescopes techniques: photometric Transit Transits
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