dc.contributorJordán, Andrés
dc.contributorBrahm Scott, Rafael
dc.date.accessioned2021-11-23T12:08:01Z
dc.date.accessioned2022-11-08T20:38:34Z
dc.date.available2021-11-23T12:08:01Z
dc.date.available2022-11-08T20:38:34Z
dc.date.created2021-11-23T12:08:01Z
dc.identifierhttps://repositorio.uai.cl//handle/20.500.12858/2796
dc.identifier10.3847/2041-8213/ab9eb9
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5148892
dc.description.abstractWe report the discovery of NGTS-11 b (=TOI-1847b), a transiting Saturn in a 35.46 day orbit around a mid K-type star (Teff = 5050 ± 80 K). We initially identified the system from a single-transit event in a TESS full-frame image light curve. Following 79 nights of photometric monitoring with an NGTS telescope, we observed a second full transit of NGTS-11 b approximately one year after the TESS single-transit event. The NGTS transit confirmed the parameters of the transit signal and restricted the orbital period to a set of 13 discrete periods. We combined our transit detections with precise radial-velocity measurements to determine the true orbital period and measure the mass of the planet. We find NGTS-11 b has a radius of 0.8170.032 0.028 RJup, a mass of 0.3440.073 0.092 MJup, and an equilibrium temperature of just 43532 34 K, making it one of the coolest known transiting gas giants. NGTS-11 b is the first exoplanet to be discovered after being initially identified as a TESS single-transit event, and its discovery highlights the power of intense photometric monitoring in recovering longer-period transiting exoplanets from single-transit events
dc.titleNGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event.
dc.typeArtículo Scopus


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