most citedTwo accreting protoplanets around the young star PDS 70

475 citations · 542 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.IM202017 cited

Diffraction-limited integral-field spectroscopy for extreme adaptive optics systems with the Multi-Core fiber-fed Integral-Field Unit

Sebastiaan Y. Haffert, Robert J. Harris, Alessio Zanutta +31

Direct imaging instruments have the spatial resolution to resolve exoplanets from their host star. This enables direct characterization of the exoplanets atmosphere, but most direc…

astro-ph.EP202013 cited

CS Cha B: A disc-obscured M-type star mimicking a polarised planetary companion

S. Y. Haffert, R. G. van Holstein, C. Ginski +6

Context. Direct imaging provides a steady flow of newly discovered giant planets and brown dwarf companions. These multi-object systems can provide information about the formation…

astro-ph.IM202037 cited

Nonlinear wavefront reconstruction with convolutional neural networks for Fourier-based wavefront sensors

Rico Landman, Sebastiaan Haffert

Fourier-based wavefront sensors, such as the Pyramid Wavefront Sensor (PWFS), are the current preference for high contrast imaging due to their high sensitivity. However, these wav…

astro-ph.EP2020

SPHERE+: Imaging young Jupiters down to the snowline

A. Boccaletti, G. Chauvin, D. Mouillet +130

SPHERE (Beuzit et al,. 2019) has now been in operation at the VLT for more than 5 years, demonstrating a high level of performance. SPHERE has produced outstanding results using a…

astro-ph.IM2020

Original use of MUSE's laser tomography adaptive optics to directly image young accreting exoplanets

Julien H. Girard, Jozua de Boer, Sebastiaan Haffert +8

We present recent results obtained with the VLT/MUSE Integral Field Spectrograph fed by the 4LGSF and its laser tomography adaptive optics module GALACSI. While this so-called narr…

astro-ph.EP2019475 cited

Two accreting protoplanets around the young star PDS 70

S. Y. Haffert, A. J. Bohn, J. de Boer +5

Newly forming proto-planets are expected to create cavities and substructures in young, gas-rich proto-planetary disks, but they are difficult to detect as they could be confused w…