activity
20172022
most citedNew constraints on the disk characteristics and companion candidates around T Cha with VLT/SPHERE

41 citations · 174 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM20211 cited

Full characterization of the instrumental polarization effects of the spectropolarimetric mode of SCExAO-CHARIS

G. J. Joost `t Hart, Rob G. van Holstein, Steven P. Bos +19

SCExAO at the Subaru telescope is a visible and near-infrared high-contrast imaging instrument employing extreme adaptive optics and coronagraphy. The instrument feeds the near-inf…

astro-ph.EP202040 cited

Dynamical Evidence of a Spiral Arm--Driving Planet in the MWC 758 Protoplanetary Disk

Bin Ren, Ruobing Dong, Rob G. van Holstein +22

More than a dozen young stars host spiral arms in their surrounding protoplanetary disks. The excitation mechanisms of such arms are under debate. The two leading hypotheses -- com…

astro-ph.EP2020

Spirals inside the millimeter cavity of transition disk SR 21

G. A. Muro-Arena, C. Ginski, C. Dominik +22

Hydrodynamical simulations of planet-disk interactions suggest that planets may be responsible for a number of the sub-structures frequently observed in disks in both scattered lig…

astro-ph.EP201921 cited

RefPlanets: Search for reflected light from extra-solar planets with SPHERE/ZIMPOL

S. Hunziker, H. M. Schmid, D. Mouillet +55

RefPlanets is a guaranteed time observation (GTO) programme that uses the Zurich IMaging POLarimeter (ZIMPOL) of SPHERE/VLT for a blind search for exoplanets in wavelengths from 60…

astro-ph.IM201918 cited

Lessons for WFIRST CGI from ground-based high-contrast systems

Vanessa P. Bailey, Michael Bottom, Eric Cady +26

The Coronagraph Instrument (CGI) for NASA's Wide Field Infrared Survey Telescope (WFIRST) will constitute a dramatic step forward for high-contrast imaging, integral field spectros…

astro-ph.EP201716 cited

Combining angular differential imaging and accurate polarimetry with SPHERE/IRDIS to characterize young giant exoplanets

Rob G. van Holstein, Frans Snik, Julien H. Girard +11

Young giant exoplanets emit infrared radiation that can be linearly polarized up to several percent. This linear polarization can trace: 1) the presence of atmospheric cloud and ha…