activity
20062023
most citedThe AstraLux Large M-dwarf Multiplicity Survey

219 citations · 1.8k across the 35 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.EPShow all

6 papers · 2 filters

astro-ph.EP2017★ 23 cited

Dynamical models to explain observations with SPHERE in planetary systems with double debris belts

C. Lazzoni, S. Desidera, F. Marzari +66

A large number of systems harboring a debris disk show evidence for a double belt architecture. One hypothesis for explaining the gap between the belts is the presence of one or mo…

astro-ph.EP2017★ 48 cited

Observability of Forming Planets and their Circumplanetary Disks I. -- Parameter Study for ALMA

J. Szulágyi, G. van der Plas, M. R. Meyer +5

We present mock observations of forming planets with ALMA. The possible detections of circumplanetary disks (CPDs) were investigated around planets of Saturn, 1, 3, 5, and 10 Jupit…

astro-ph.EP2017★ 14 cited

High signal-to-noise spectral characterization of the planetary-mass object HD 106906 b

Sebastian Daemgen, Kamen Todorov, Sascha P. Quanz +4

We spectroscopically characterize the atmosphere of HD 106906b, a young low-mass companion near the deuterium burning limit. The wide separation from its host star of 7.1" makes it…

astro-ph.EP2017★ 19 cited

Orbiting a binary: SPHERE characterisation of the HD 284149 system

Mariangela Bonavita, V. D'Orazi, D. Mesa +52

In this paper we present the results of the SPHERE observation of the HD 284149 system, aimed at a more detailed characterisation of both the primary and its brown dwarf companion.…

astro-ph.EP2017★ 205 cited

Discovery of a warm, dusty giant planet around HIP65426

G. Chauvin, S. Desidera, A. -M. Lagrange +120

The SHINE program is a large high-contrast near-infrared survey of 600 young, nearby stars. It is aimed at searching for and characterizing new planetary systems using VLT/SPHERE's…

astro-ph.EP2017★ 41 cited

New constraints on the disk characteristics and companion candidates around T Cha with VLT/SPHERE

A. Pohl, E. Sissa, M. Langlois +34

The transition disk around the T Tauri star T Cha possesses a large gap, making it a prime target for high-resolution imaging in the context of planet formation. We aim to find sig…