activity
20142024
most citedThe VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits: II- Survey description, results and performances

118 citations · 549 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2024

The SPHERE view of the Taurus star-forming region

A. Garufi, C. Ginski, R. G. van Holstein +31

The sample of planet-forming disks observed by high-contrast imaging campaigns over the last decade is mature enough to enable the demographical analysis of individual star-forming…

astro-ph.GA20241 cited

The SPHERE view of the Chamaeleon I star-forming region

C. Ginski, A. Garufi, M. Benisty +32

We used VLT/SPHERE to observe 20 systems in the Cha I cloud in polarized scattered light in the near-infrared. We combined the scattered light observations with existing literature…

astro-ph.SR2024

The discovery of two new benchmark brown dwarfs with precise dynamical masses at the stellar-substellar boundary

Emily L. Rickman, Will Ceva, Elisabeth C. Matthews +7

Aims. Measuring dynamical masses of substellar companions is a powerful tool to test models of mass-luminosity-age relations, as well as determining observational features that con…

astro-ph.EP20236 cited

TOI-858 B b: A hot Jupiter on a polar orbit in a loose binary

J. Hagelberg, L. D. Nielsen, O. Attia +30

We report the discovery of a hot Jupiter on a 3.28-day orbit around a 1.08 M G0 star that is the secondary component in a loose binary system. Based on follow-up radial vel…

astro-ph.EP202318 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.EP202325 cited

TOI-5678 b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS

S. Ulmer-Moll, H. P. Osborn, A. Tuson +92

A large sample of long-period giant planets has been discovered thanks to long-term radial velocity surveys, but only a few dozen of these planets have a precise radius measurement…