activity
20152026
most citedDiscovery of a warm, dusty giant planet around HIP65426

205 citations · 1.8k across the 64 of their papers we have counts for

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Showing 2018Show all

13 papers · 1 filter

astro-ph.EP2018

A search for accreting young companions embedded in circumstellar disks: High-contrast H imaging with VLT/SPHERE

G. Cugno, S. P. Quanz, S. Hunziker +37

Aims: We want to detect and quantify observables related to accretion processes occurring locally in circumstellar disks, which could be attributed to young forming planets. We foc…

astro-ph.EP2018

Comprehensive analysis of HD 105, a young Solar System analog

J. P. Marshall, J. Milli, É. Choquet +5

HD~105 is a nearby, pre-main sequence G0 star hosting a moderately bright debris disc (). HD~105 and its surroundings might therefore…

astro-ph.IM2018

Origin of the asymmetry of the wind driven halo observed in high contrast images

F. Cantalloube, E Por, K. Dohlen +9

The latest generation of high contrast instruments dedicated to exoplanets and circumstellar disks imaging are equipped with extreme adaptive optics and coronagraphs to reach contr…

astro-ph.IM2018

SPHERE / ZIMPOL high resolution polarimetric imager. I. System overview, PSF parameters, coronagraphy, and polarimetry

H. M. Schmid, A. Bazzon, R. Roelfsema +59

We describe the Zurich Imaging Polarimeter (ZIMPOL), the visual focal plane subsystem of the SPHERE "VLT planet finder", which pushes the limits of current AO systems to shorter wa…

astro-ph.IM2018

Low Wind Effect on VLT/SPHERE : impact, mitigation strategy, and results

Julien Milli, Markus Kasper, Pierre Bourget +14

The low wind effect is a phenomenon disturbing the phase of the wavefront in the pupil of a large telescope obstructed by spiders, in the absence of wind. It can be explained by th…

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…