Ground-based light curve follow-up validation observations of TESS object of interest TOI 5356.01

Abstract

Context: The current definition of an exoplanet is changing the more we learn about them. Several exoplanet detection missions have been launched over the years since the first one was discovered, each using different detection methods with the most successful one being the transit method. Detecting exoplanets does not always mean they are confirmed, and they must be checked and reviewed to determine their existence. Aims: The goal of this paper is to present the results of a follow up observation of the exoplanet candidate: 5356.01. The observation and conclusion help to build upon our definition of an exoplanet and how they form.