activity
20052026
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 10.6k across the 208 of their papers we have counts for

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Showing 2013Show all

13 papers · 1 filter

astro-ph.SR2013★ 239 cited

Structures in the protoplanetary disk of HD142527 seen in polarized scattered light

Henning Avenhaus, Sascha P. Quanz, Hans Martin Schmid +4

We present H- and Ks-band polarized differential images (PDI) of the Herbig Ae/Be star HD142527, revealing its optically thick outer disk and the nearly empty gap. The very small i…

astro-ph.EP2013★ 179 cited

Small vs large dust grains in transitional disks: do different cavity sizes indicate a planet?

Antonio Garufi, Sascha P Quanz, Henning Avenhaus +7

Transitional disks represent a short stage of the evolution of circumstellar material. Studies of dust grains in these objects can provide pivotal information on the mechanisms of…

astro-ph.EP2013★ 45 cited

Optimized Principal Component Analysis on Coronagraphic Images of the Fomalhaut System

T. Meshkat, M. Kenworthy, S. P. Quanz +1

We present the results of a study to optimize the principal component analysis (PCA) algorithm for planet detection, a new algorithm complementing ADI and LOCI for increasing the c…

astro-ph.EP2013★ 130 cited

Confirmation of the planet around HD 95086 by direct imaging

J. Rameau, G. Chauvin, A. -M. Lagrange +8

VLT/NaCo angular differential imaging at L' (3.8 microns) revealed a probable giant planet comoving with the young and early-type HD 95086 also known to harbor an extended debris d…

astro-ph.EP2013★ 76 cited

Multiple spiral patterns in the transitional disk of HD 100546

A. Boccaletti, E. Pantin, A. -M. Lagrange +3

Protoplanetary disks around young stars harbor many structures related to planetary formation. Of particular interest, spiral patterns were discovered among several of these disks…

astro-ph.EP2013★ 13 cited

On the frequency of planetary systems around G-dwarfs

Richard J. Parker, Sascha P. Quanz

We determine the fraction of G-dwarf stars that could host stable planetary systems based on the observed properties of binaries in the Galactic field, and in various postulated pr…