activity
20172020
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 469 across the 9 of their papers we have counts for

collaborators

17 papers

astro-ph.EP202027 cited

The search for disks or planetary objects around directly imaged companions: A candidate around DH Tau B

C. Lazzoni, A. Zurlo, S. Desidera +45

In recent decades, thousands of substellar companions have been discovered with both indirect and direct methods of detection. In this paper, we focus our attention on substellar c…

astro-ph.EP202026 cited

Orbital and spectral characterization of the benchmark T-type brown dwarf HD 19467B

A. -L. Maire, K. Molaverdikhani, S. Desidera +42

Context. Detecting and characterizing substellar companions for which the luminosity, mass, and age can be determined independently is of utter importance to test and calibrate the…

astro-ph.EP2020

SPHERE+: Imaging young Jupiters down to the snowline

A. Boccaletti, G. Chauvin, D. Mouillet +130

SPHERE (Beuzit et al,. 2019) has now been in operation at the VLT for more than 5 years, demonstrating a high level of performance. SPHERE has produced outstanding results using a…

astro-ph.EP201924 cited

A dusty benchmark brown dwarf near the ice line of HD 72946

A. -L. Maire, J. -L. Baudino, S. Desidera +12

Context. HD72946 is a bright and nearby solar-type star hosting a low-mass companion at long period (P~16 yr) detected with the radial velocities (RV) method. The companion has a m…

astro-ph.EP201984 cited

VLT/SPHERE exploration of the young multiplanetary system PDS70

D. Mesa, M. Keppler, F. Cantalloube +51

Context. PDS 70 is a young (5.4 Myr), nearby (~113 pc) star hosting a known transition disk with a large gap. Recent observations with SPHERE and NACO in the near-infrared (NIR) al…

astro-ph.EP2019

Toward the Analysis of JWST Exoplanet Spectra: the effective temperature in the context of direct imaging

Jean-Loup Baudino, J. Taylor, P. G. J. Irwin +1

The current sparse wavelength range coverage of exoplanet direct imaging observations, and the fact that models are defined using a finite wavelength range, lead both to uncertaint…