One of the main goals of the NASA Transiting Exoplanet Survey Satellite (TESS) mission is the discovery of Earth-like planets around nearby M-dwarf stars. We present the discovery and validation of three new short-period Earth-sized planets orbiting nearby M dwarfs: TOI-5720 b, TOI-6008 b, and TOI-6086 b. We combined TESS data, ground-based multicolor light curves, ground-based optical and near-infrared spectroscopy, and Subaru/IRD radial velocity data to validate the planetary candidates and constrain the physical parameters of the systems. In addition, we used archival images, high-resolution imaging, and statistical validation techniques to support the planetary validation.
Three short-period Earth-sized planets around M dwarfs discovered by TESS: TOI-5720 b, TOI-6008 b, and TOI-6086 b / Barkaoui, K., Schwarz, R.P., Narita, N., Mistry, P., Magliano, C., Hirano, T., Maity, M., Burgasser, A.J., Rackham, B.V., Murgas, F., Pozuelos, F.J., Stassun, K.G., Everett, M.E., Ciardi, D.R., Lamman, C., Pass, E.K., Bieryla, A., Aganze, C., Esparza-Borges, E., Collins, K.A., et al.. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 0004-6361. - 687:(2024). [10.1051/0004-6361/202349127]
Three short-period Earth-sized planets around M dwarfs discovered by TESS: TOI-5720 b, TOI-6008 b, and TOI-6086 b
Magliano, C.;Covone, G.;
2024
Abstract
One of the main goals of the NASA Transiting Exoplanet Survey Satellite (TESS) mission is the discovery of Earth-like planets around nearby M-dwarf stars. We present the discovery and validation of three new short-period Earth-sized planets orbiting nearby M dwarfs: TOI-5720 b, TOI-6008 b, and TOI-6086 b. We combined TESS data, ground-based multicolor light curves, ground-based optical and near-infrared spectroscopy, and Subaru/IRD radial velocity data to validate the planetary candidates and constrain the physical parameters of the systems. In addition, we used archival images, high-resolution imaging, and statistical validation techniques to support the planetary validation.| File | Dimensione | Formato | |
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