activity
20172024
most citedHD142527: Quantitative disk polarimetry with SPHERE

36 citations · 104 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2024★ 3 cited

A solar rotation signature in cosmic dust: frequency analysis of dust particle impacts on the Wind spacecraft

Lennart R. Baalmann, Silvan Hunziker, Arthur Péronne +7

Dust particle impacts on the Wind spacecraft were detected with its plasma wave instrument Wind/WAVES. Frequency analysis on this dust impact time series revealed spectral peaks in…

astro-ph.IM2023★ 7 cited

Synergies between interstellar dust and heliospheric science with an Interstellar Probe

Veerle J. Sterken, Silvan Hunziker, Kostas Dialynas +40

We discuss the synergies between heliospheric and dust science, the open science questions, the technological endeavors and programmatic aspects that are important to maintain or d…

astro-ph.EP2021★ 36 cited

HD142527: Quantitative disk polarimetry with SPHERE

S. Hunziker, H. M. Schmid, J. Ma +17

We present high-precision photometry and polarimetry for the protoplanetary disk around HD142527, with a focus on determining the light scattering parameters of the dust. We re-red…

astro-ph.GA2021★ 2 cited

High angular resolution polarimetric imaging of the nucleus of NGC 1068: Disentangling the polarising mechanisms

L. Grosset, D. Rouan, F. Marin +8

Polarisation is a decisive method to study the inner region of active galactic nuclei (AGNs) since it is not affected by contrast issues similarly to how classical imaging is. When…

astro-ph.EP2019★ 21 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.IM2017★ 35 cited

A PCA-based approach for subtracting thermal background emission in high-contrast imaging data

Silvan Hunziker, Sascha P. Quanz, Adam Amara +1

Ground-based observations at thermal infrared wavelengths suffer from large background radiation due to the sky, telescope and warm surfaces in the instrument. This significantly l…