dc.creatorLendl, Monika
dc.creatorBouchy, Françoise
dc.creatorGill, Samuel
dc.creatorNielsen, Louise D.
dc.creatorTurner, Oliver
dc.creatorStassun, Keivan
dc.creatorActon, Jack S.
dc.creatorAnderson, David R.
dc.creatorArmstrong, David J.
dc.creatorBayliss, Daniel
dc.creatorBelardi, Claudia
dc.creatorBryant, Edward M.
dc.creatorBurleigh, Matthew R.
dc.creatorChaushev, Alexander
dc.creatorCasewell, Sarah L.
dc.creatorCooke, Benjamin F
dc.creatorEigmüller, Philipp
dc.creatorGillen, Edward
dc.creatorGoad, Michael R.
dc.creatorGünther, Maximilian N.
dc.creatorHagelberg, Janis
dc.creatorJenkins, James S.
dc.creatorLouden, Tom
dc.creatorMarmier, Maxime
dc.creatorMcCormac, James
dc.creatorMoyano, Maximiliano
dc.creatorPollacco, Don
dc.creatorRaynard, Liam
dc.creatorTilbrook, Rosanna H.
dc.creatorUdry, Stéphane
dc.creatorVines, José I.
dc.creatorWest, Richard G.
dc.creatorWheatley, Peter J.
dc.creatorRicker, George
dc.creatorVanderspek, Roland
dc.creatorLatham, David W.
dc.creatorSeager, Sara
dc.creatorWinn, Josh
dc.creatorJenkins, Jon M.
dc.creatorAddison, Brett
dc.creatorBriceño, César
dc.creatorBrahm, Rafael
dc.creatorCaldwell, Douglas A.
dc.creatorDoty, John
dc.creatorEspinoza, Néstor
dc.creatorGoeke, Bob
dc.creatorHenning, Thomas
dc.creatorJordán, Andrés
dc.creatorKrishnamurthy, Akshata
dc.creatorLaw, Nicholas
dc.creatorMorris, Robert
dc.creatorOkumura, Jack
dc.creatorMann, Andrew W.
dc.creatorRodriguez, Joseph E.
dc.creatorSarkis, Paula
dc.creatorSchlieder, Joshua
dc.creatorTwicken, Joseph D.
dc.creatorVillanueva, Steven
dc.creatorWittenmyer, Robert A.
dc.creatorWright, Duncan J.
dc.creatorZiegler, Carl
dc.date.accessioned2020-05-18T20:59:29Z
dc.date.available2020-05-18T20:59:29Z
dc.date.created2020-05-18T20:59:29Z
dc.date.issued2020
dc.identifierMNRAS, Vol. 492, No.2, (2020), 1761–1769
dc.identifier10.1093/mnras/stz3545
dc.identifierhttps://repositorio.uchile.cl/handle/2250/174794
dc.description.abstractWe report the period, eccentricity, and mass determination for the Transiting Exoplanet Survey Satellite (TESS) single-transit event candidate TOI-222, which displayed a single 3000 ppm transit in the TESS 2-min cadence data from Sector 2. We determine the orbital period via radial velocity measurements (P = 33.9 d), which allowed for ground-based photometric detection of two subsequent transits. Our data show that the companion to TOI-222 is a low-mass star, with a radius of 0.18(-0.10)(+0.39) R-circle dot and a mass of 0.23 +/- 0.01 M-circle dot. This discovery showcases the ability to efficiently discover long-period systems from TESS single-transit events using a combination of radial velocity monitoring coupled with high-precision ground-based photometry.
dc.languageen
dc.publisherOxford Unv Press
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectTechniques: photometric
dc.subjectStars: individual: TOI-222
dc.subjectPlanetary systems
dc.titleTOI-222: a single-transit TESS candidate revealed to be a 34-day eclipsing binary with CORALIE, EulerCam and NGTS
dc.typeArtículo de revista


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