activity
19982023
most citedDiscovery of a Low-Mass Brown Dwarf Companion of the Young Nearby Star G196-3

156 citations · 205 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2023

Photometric follow-up of the 20 Myr-old multi-planet host star V1298~Tau with CHEOPS and ground-based telescopes

M. Damasso, G. Scandariato, V. Nascimbeni +25

V1298 Tau hosts at least four planets. Since its discovery, this system has been a target of intensive photometric and spectroscopic monitoring. The characterisation of its archite…

astro-ph.SR2023★ 13 cited

Young nearby open clusters and their luminosity functions

M. Žerjal, N. Lodieu, A. Pérez-Garrido +3

Context. Open clusters are groups of coeval stars sharing properties such as distance and metallicity, and they are key to understanding stellar evolution. Aims. Our main goal is t…

astro-ph.EP2023★ 18 cited

The GAPS program at TNG XLVII: The unusual formation history of V1298 Tau

D. Turrini, F. Marzari, D. Polychroni +33

Observational data from space and ground-based campaigns reveal that the 10-30 Ma old V1298 Tau star hosts a compact and massive system of four planets. Mass estimates for the two…

astro-ph.SR2023★ 9 cited

The cosmic waltz of Coma Berenices and Latyshev 2 (Group X). Membership, phase-space structure, mass, and energy distributions

J. Olivares, N. Lodieu, V. J. S. Béjar +3

Context. Open clusters (OCs) are fundamental benchmarks where theories of star formation and stellar evolution can be tested and validated. Coma Ber and Latyshev 2 (Group X) are th…

astro-ph.SR2020

Two close binaries across the hydrogen-burning limit in the Praesepe open cluster

N. Lodieu, C. del Burgo, E. Manjavacas +7

We present Keck I/OSIRIS and Keck II/NIRC2 adaptive optics imaging of two member candidates of the Praesepe stellar cluster (d=186.180.11 pc; 590-790 Myr), UGC J08451066+21481…

astro-ph.GA2017★ 8 cited

Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes

M. Marks, E. L. Martín, V. J. S. Béjar +6

Whether BDs form as stars through gravitational collapse ("star-like") or BDs and some very low-mass stars constitute a separate population which form alongside stars comparable to…