Null transit detections of 68 radial velocity exoplanets observed by TESS
F. V. Lovos (1, 2), R. F. D\'iaz (2, 3), and L. A. Nieto (3 and, 4) ((1) Universidad Nacional de C\'ordoba, Observatorio Astron\'omico,, C\'ordoba, Argentina, (2) Consejo Nacional de Investigaciones Cient\'ificas y, T\'ecnicas (CONICET), CABA, Argentina

TL;DR
This study used TESS data to search for transits of 68 RV-detected exoplanets, finding no new transits and confirming the non-transiting nature of most, which helps refine their physical characteristics.
Contribution
First systematic search for transits of RV-detected exoplanets with TESS, providing constraints on their sizes and transit probabilities.
Findings
No new transits detected among 68 planets.
Excluded planets larger than 2.4 Earth radii assuming central transits.
Confirmed two known transiting planets in the sample.
Abstract
In recent years the number of exoplanets has grown considerably. The most successful techniques in these detections are the radial velocity (RV) and planetary transits techniques, the latter significantly advanced by the Kepler, K2 and, more recently, the TESS missions. The detection of exoplanets both by means of transit and by RVs is of importance, because this would allows characterizing their bulk densities, and internal compositions. The Transiting Exoplanet Survey Satellite (TESS) survey offers a unique possibility to search for transits of extrasolar planets detected by RV. In this work, we present the results of the search for transits of planets detected with the radial velocity technique, using the photometry of the TESS space mission. We focus on systems with super-Earths and Neptunes planets on orbits with periods shorter than 30 days. This cut is intended to keep objects…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation
