Baptiste Cecconi

TL;DR: The proceedings of the homonymous international conference on all aspects of impact cratering and planetary science, which was held in October 2019 in Brasília, Brazil, contained a sizable suite of contributions dealing with regional impact records (Australia, Sweden), impact craters and impactites, early Archean impacts and geophysical characteristics of impact structures, shock metamorphic investigations, post-impact hydrothermalism, and structural geology and morphometry of impact structure as discussed by the authors.

TL;DR: In this paper, the authors used a more extensive set of data than the original study to confirm the correlation of higher occurrence probability of SKR when Titan is located near local midnight and used the direction finding capability of the Cassini Radio Plasma Wave instrument (RPWS) to determine if this radio emission emanates from particular source regions.

TL;DR: VESPA encompasses a wide scope, including surfaces, atmospheres, magnetospheres and planetary plasmas, small bodies, heliophysics, exoplanets, and spectroscopy in solid phase, and relies in particular on standards and tools developed for the Astronomy VO (IVOA) and extends them where required to handle specificities of Solar System studies.

TL;DR: NenuFAR as mentioned in this paper is a new radio telescope developed and built on the site of the Nancay Radio Observatory, which is designed to observe the largely unexplored frequency window from 10 to 85 GHz, offering a high sensitivity across its full bandwidth.

TL;DR: A survey of electrostatic electron cyclotron harmonic (ECH) emissions observed at Saturn by the radio and plasma wave science (RPWS) investigation on board the Cassini spacecraft is presented in this paper.