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20162026
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 2.1k across the 64 of their papers we have counts for

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Showing 2018 · astro-ph.EPShow all

9 papers · 2 filters

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

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

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

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

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.EP2018

Orbital and spectral analysis of the benchmark brown dwarf HD 4747B

S. Peretti, D. Ségransan, B. Lavie +43

The study of high contrast imaged brown dwarfs and exoplanets depends strongly on evolutionary models. To estimate the mass of a directly imaged substellar object, its extracted ph…