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20142026
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 4.2k across the 85 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.EP2018★ 52 cited

Spectral and orbital characterisation of the directly imaged giant planet HIP 65426 b

A. C. Cheetham, M. Samland, S. S. Brems +38

HIP 65426 b is a recently discovered exoplanet imaged during the course of the SPHERE-SHINE survey. Here we present new and observations of the planet from the NACO instr…

astro-ph.EP2018★ 42 cited

High-Contrast study of the candidate planets and protoplanetary disk around HD~100546

E. Sissa, R. Gratton, A. Garufi +62

The nearby Herbig Be star HD100546 is known to be a laboratory for the study of protoplanets and their relation with the circumstellar disk that is carved by at least 2 gaps. We ob…

astro-ph.EP2018★ 700 cited

Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70

M. Keppler, M. Benisty, A. Müller +123

Young circumstellar disks are of prime interest to understand the physical and chemical conditions under which planet formation takes place. Only very few detections of planet cand…

astro-ph.EP2018★ 80 cited

The GJ 504 system revisited. Combining interferometric, radial velocity, and high contrast imaging data

M. Bonnefoy, K. Perraut, A. -M. Lagrange +79

The G-type star GJ504A is known to host a 3 to 35 MJup companion whose temperature, mass, and projected separation all contribute to make it a test case for the planet formation th…

astro-ph.EP2018★ 263 cited

Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk

A. Müller, M. Keppler, Th. Henning +43

Aims: We aim to characterize the orbital and atmospheric properties of PDS 70 b, which was first identified on May 2015 in the course of the SHINE survey with SPHERE, the extreme a…

astro-ph.SR2018★ 20 cited

Dynamical masses of M-dwarf binaries in young moving groups: I - The case of TWA 22 and GJ 2060

L. Rodet, M. Bonnefoy, S. Durkan +48

Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less reliable at young ages ( 200 Myr) and i…