NGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event
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2020Metadata
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Gill, Samuel
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NGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event
Author
- Gill, Samuel;
- Wheatley, Peter J.;
- Cooke, Benjamin F;
- Jordán, Andrés;
- Nielsen, Louise D.;
- Bayliss, Daniel;
- Anderson, David R.;
- Vines, José I.;
- Lendl, Monika;
- Acton, Jack S.;
- Armstrong, David J.;
- Bouchy, François;
- Brahm, Rafael;
- Bryant, Edward M.;
- Burleigh, Matthew R.;
- Casewell, Sarah L.;
- Eigmüller, Philipp;
- Espinoza, Néstor;
- Gillen, Edward;
- Goad, Michael R.;
- Grieves, Nolan;
- Günther, Maximilian N.;
- Henning, Thomas;
- Hobson, Melissa J.;
- Hogan, Aleisha;
- Jenkins, James S.;
- McCormac, James;
- Moyano, Maximiliano;
- Osborn, Hugh P.;
- Pollacco, Don;
- Queloz, Didier;
- Rauer, Heike;
- Raynard, Liam;
- Lagos Rojas, Felipe Alejandro;
- Sarkis, Paula;
- Smith, Alexis M. S.;
- Tala Pinto, Marcelo;
- Tilbrook, Rosanna H.;
- Udry, Stéphane;
- Watson, Christopher A.;
- West, Richard G.;
Abstract
We report the discovery of NGTS-11 b (=TOI-1847b), a transiting Saturn in a 35.46 day orbit around a mid K-type star (T-eff = 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 +/-(0.028)(0.032) R-Jup, a mass of 0.344 +/-(0.092)(0.073) M-Jup, and an equilibrium temperature of just 435 +/-(34)(32) 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.
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The Astrophysical Journal Letters, 898:L11 (6pp), 2020 July 20
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