TOI-222: a single-transit TESS candidate revealed to be a 34-d eclipsing binary with CORALIE, EulerCam, and NGTS
dc.contributor.author | Lendl, M. | |
dc.contributor.author | Bouchy, F. | |
dc.contributor.author | Gill, S. | |
dc.contributor.author | Nielsen, L. D. | |
dc.contributor.author | Turner, O. | |
dc.contributor.author | Stassun, K. | |
dc.contributor.author | Acton, J. S. | |
dc.contributor.author | Anderson, D. R. | |
dc.contributor.author | Armstrong, D. J. | |
dc.contributor.author | Bayliss, D. | |
dc.contributor.author | Belardi, C. | |
dc.contributor.author | Bryant, E. M. | |
dc.contributor.author | Burleigh, M. R. | |
dc.contributor.author | Chaushev, A. | |
dc.contributor.author | Casewell, S. L. | |
dc.contributor.author | Cooke, B. F. | |
dc.contributor.author | Eigmüller, P. | |
dc.contributor.author | Gillen, E. | |
dc.contributor.author | Goad, M. R. | |
dc.contributor.author | Gunther, M. N. | |
dc.contributor.author | Hagelberg, J. | |
dc.contributor.author | Jenkins, J. S. | |
dc.contributor.author | Louden, T. | |
dc.contributor.author | Marmier, M. | |
dc.contributor.author | McCormac, J. | |
dc.contributor.author | Moyano, M. | |
dc.contributor.author | Pollacco, D. | |
dc.contributor.author | Raynard, L. | |
dc.contributor.author | Tilbrook, R. H. | |
dc.contributor.author | Udry, S. | |
dc.contributor.author | Vines, J. I. | |
dc.contributor.author | West, R. G. | |
dc.contributor.author | Wheatley, P. J. | |
dc.contributor.author | Ricker, G. | |
dc.contributor.author | Vanderspek, R. | |
dc.contributor.author | Latham, D. W. | |
dc.contributor.author | Seager, S. | |
dc.contributor.author | Winn, J. | |
dc.contributor.author | Jenkins, J. M. | |
dc.contributor.author | Addison, B. | |
dc.contributor.author | Briceño, C. | |
dc.contributor.author | Brahm, R. | |
dc.contributor.author | Caldwell, D. A. | |
dc.contributor.author | Doty, J. | |
dc.contributor.author | Espinoza, N. | |
dc.contributor.author | Goeke, B. | |
dc.contributor.author | Henning, T. | |
dc.contributor.author | Jordán, A. | |
dc.contributor.author | Krishnamurthy, A. | |
dc.contributor.author | Law, N. | |
dc.contributor.author | Morris, R. | |
dc.contributor.author | Okumura, J. | |
dc.contributor.author | Mann, A. W. | |
dc.contributor.author | Rodriguez, J. E. | |
dc.contributor.author | Sarkis, P. | |
dc.contributor.author | Schlieder, J. | |
dc.contributor.author | Twicken, J. D. | |
dc.contributor.author | Villanueva, S. | |
dc.contributor.author | Wittenmyer, R. A. | |
dc.contributor.author | Wright, D. J. | |
dc.contributor.author | Ziegle, C. | |
dc.date.accessioned | 2022-05-24T14:48:09Z | |
dc.date.available | 2022-05-24T14:48:09Z | |
dc.date.issued | 2019 | |
dc.description.abstract | We 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⊙ and a mass of 0.23 ± 0.01 M⊙. 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.fechaingreso.objetodigital | 2025-03-13 | |
dc.format.extent | 1769 páginas | |
dc.fuente.origen | OUP | |
dc.identifier.doi | 10.1093/mnras/stz3545 | |
dc.identifier.eissn | 1365-2966 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.uri | https://doi.org/10.1093/mnras/stz3545 | |
dc.identifier.uri | https://ieeexplore.ieee.org/stamp/stamp.jsp?arnumber=9114000 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/64268 | |
dc.identifier.wosid | WOS:000512297600016 | |
dc.information.autoruc | Instituto de física ; Brahm Scott, Rafael ; S/I ; 162088 | |
dc.issue.numero | 1 | |
dc.language.iso | en | |
dc.nota.acceso | contenido parcial | |
dc.pagina.final | 1769 | |
dc.pagina.inicio | 1761 | |
dc.revista | Monthly Notices of the Royal Astronomical Society | |
dc.rights | acceso restringido | |
dc.subject | Techniques: photometric | |
dc.subject | Stars: individual :TOI-222 | |
dc.subject | Planetary systems | |
dc.subject.dewey | Astronomía | |
dc.subject.ods | 13 Climate action | |
dc.subject.odspa | 13 Acción por el clima | |
dc.subject.other | Estrellas binarias eclipsantes | |
dc.subject.other | Planetas - Orbitas | |
dc.subject.other | Planetas extrasolares | |
dc.title | TOI-222: a single-transit TESS candidate revealed to be a 34-d eclipsing binary with CORALIE, EulerCam, and NGTS | es_ES |
dc.type | artículo | |
dc.volumen | 492 | |
sipa.codpersvinculados | 162088 |
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