Characterising transiting exoplanets at long orbital period: lessons learned for PLATO from 10 years of monitoring the HIP41378 system

arXiv:2606.22996 · astro-ph.EP, astro-ph.IM · Submitted 2026-06-22 · Read on arXiv

Alexandre Santerne, Salomé Grouffal, Stéphane Udry

astro-ph.EP, astro-ph.IM

Submitted: 2026-06-22

Comments: Accepted for publication in The ESO Messenger

License: http://creativecommons.org/licenses/by/4.0/

The gist: The upcoming launch of the PLATO mission will open a new area of exoplanetary research by probing transiting exoplanets at long orbital periods around bright stars.

Abstract

The upcoming launch of the PLATO mission will open a new area of exoplanetary research by probing transiting exoplanets at long orbital periods around bright stars. These planets will be amenable to follow-up observations, especially with the ESO telescopes as the first PLATO field is in the southern sky. In this paper we listed the lessons we learned by monitoring the bright HIP41378 multi-planetary system over one decade via both radial-velocity and transit observations. These lessons are important for the follow-up strategy of PLATO transiting exoplanets.

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