Now showing items 1-5 of 5

    • Jones, M. I.; Brahm, R.; Espinoza, N.; Jordán, A.; Rojas, F.; Rabus, M.; Drass, H.; Zapata, A.; Soto, M. G.; Jenkins, James Stewart; Vuckovic, M.; Ciceri, S.; Sarkis, P. (EDP Sciences, 2018)
      Although the majority of radial velocity detected planets have been found orbiting solar-type stars, a fraction of them have been discovered around giant stars. These planetary systems have revealed different orbital ...
    • Jones, M. I.; Brahm, R.; Espinoza N., Arturo; Jordán, A.; Rojas, F.; Rabus, M.; Drass, H.; Zapata, A.; Soto, M. G.; Jenkins, James Stewart; Vuckovic, M.; Ciceri, S.; Sarkis, P. (EDP Sciences, 2018)
      Although the majority of radial velocity detected planets have been found orbiting solar-type stars, a fraction of them have been discovered around giant stars. These planetary systems have revealed different orbital ...
    • Bouma, L. G.; Hartman, J. D.; Brahm, R.; Evans, P.; Collins, K. A.; Zhou, G.; Sarkis, P.; Quinn, S. N.; Leon, J. de; Livingston, J.; Bergmann, C.; Stassun, K. G.; Bhatti, W.; Winn, J. N.; Bakos, G. A.; Abe, L.; Crouzet, N.; Dransfield, G.; Guillot, T.; Marie-Sainte, W.; Mekarnia, D.; Triaud, A. H. M. J.; Tinney, C. G.; Henning, T.; Espinoza N., Arturo; Jordan, A.; Barbieri, M. A.; Nandakumar, S.; Trifonov, T.; Vines, J. I.; Vuckovic, M.; Ziegler, C.; Law, N.; Mann, A. W.; Ricker, G. R.; Vanderspek, R.; Seager, S.; Jenkins, J. M.; Burke, C. J.; Dragomir, D.; Levine, A. M.; Quintana, E. V.; Rodríguez, J. E.; Smith, J. C.; Wohler, B. (IOP Publishing, 2020)
      We report the discovery of TOI 837b and its validation as a transiting planet. We characterize the system using data from the NASA Transiting Exoplanet Survey Satellite mission, the ESA Gaia mission, ground-based photometry ...
    • Brahm, R.; Espinoza, N.; Jordan, A.; Rojas, F.; Sarkis, P.; Díaz, M. R; Rabus, M.; Drass, H.; Lachaume, R.; Soto, M. G.; Jenkins, James Stewart; Jones, M. I.; Henning, Thomas; Pantoja, B.; Vuckovic, M. (Oxford University Press, 2018-06)
      We report the discovery of K2-232 b using photometric data of the Kepler K2 satellite coupled with ground-based spectroscopic observations. K2-232 b has a mass of M-P = 0.397 +/- 0.037 M-J, a radius of R-P = 1.00 +/- 0.020 ...
    • Bluhm, P.; Jones, M. I.; Vanzi, L.; Soto, M. G; Vos, J.; Wittenmyer, R. A.; Drass, H.; Jenkins, James Stewart; Olivares, F.; Mennickent, R. E.; Vuckovic, M.; Rojo, P.; Melo, C. H. F. (EDP Sciences, 2016)
      We report the discovery of 24 spectroscopic binary companions to giant stars. We fully constrain the orbital solution for 6 of these systems. We cannot unambiguously derive the orbital elements for the remaining stars ...