most citedExploring dust around HD142527 down to 0.025" / 4au using SPHERE/ZIMPOL

100 citations · 397 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP201793 cited

The circumstellar disk HD169142: gas, dust and planets acting in concert?

A. Pohl, M. Benisty, P. Pinilla +33

HD169142 is an excellent target to investigate signs of planet-disk interaction due to the previous evidence of gap structures. We performed J-band (~1.2μm) polarized intensity…

astro-ph.EP201718 cited

Three years of SPHERE: the latest view of the morphology and evolution of protoplanetary discs

Antonio Garufi, Myriam Benisty, Tomas Stolker +11

Spatially resolving the immediate surroundings of young stars is a key challenge for the planet formation community. SPHERE on the VLT represents an important step forward by incre…

astro-ph.EP201769 cited

Variable dynamics in the inner disk of HD 135344B revealed with multi-epoch scattered light imaging

Tomas Stolker, Mike Sitko, Bernard Lazareff +12

We present multi-epoch VLT/SPHERE observations of the protoplanetary disk around HD 135344B (SAO 206462). The -band scattered light imagery reveal, with high spatial resolution…

astro-ph.EP201776 cited

Investigation of the inner structures around HD169142 with VLT/SPHERE

R. Ligi, A. Vigan, R. Gratton +47

We present observations of the Herbig Ae star HD169142 with VLT/SPHERE instruments InfraRed Dual-band Imager and Spectrograph (IRDIS) ( and bands) and the Integral Fie…

astro-ph.EP2017100 cited

Exploring dust around HD142527 down to 0.025" / 4au using SPHERE/ZIMPOL

H. Avenhaus, S. P. Quanz, H. M. Schmid +25

We have observed the protoplanetary disk of the well-known young Herbig star HD 142527 using ZIMPOL Polarimetric Differential Imaging with the VBB (Very Broad Band, ~600-900nm) fil…

astro-ph.EP201741 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…