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Discovery of a warm, dusty giant planet around HIP 65426
(EDP Sciences, 2017)
Aims. The SHINE program is a high-contrast near-infrared survey of 600 young, nearby stars aimed at searching for and characterizing new planetary systems using VLT/SPHERE's unprecedented high-contrast and high-angular-resolution ...
Self-adjusting data acquisition system for Low Layer SCIDAR
(Monthly Notices of the Royal Astronomical Society, 2012)
New constraints on the dust surrounding HR 4796A
(ESO, 2015)
Context. HR 4796A is surrounded by a well-structured and very bright circumstellar disc shaped like an annulus with many interesting features: very sharp inner and outer edges, brightness asymmetries, centre offset, and ...
Potential and sky coverage for off-axis fringe tracking in optical long baseline interferometry
(Oxford, 2021)
The spectacular results provided by the second-generationVLTI instruments GRAVITY and MATISSE on active galactic nuclei (AGN) trigger and justify a strong increase in the sensitivity limit of optical interferometers. A key ...
HD 169142 in the eyes of ZIMPOL/SPHERE
(Oxford University Press, 2018)
We present new data of the protoplanetary disc surrounding the Herbig Ae/Be star HD 169142 obtained in the very broad-band (VBB) with the Zurich imaging polarimeter (ZIMPOL), a sub-system of the Spectro-Polarimetric ...
The inner environment of Z Canis Majoris: High-contrast imaging polarimetry with NaCo
(EDP SCIENCES, 2015)
Context. Z CMa is a binary composed of an embedded Herbig Be and an FU Ori class star separated by ∼100 au. Observational
evidence indicates a complex environment in which each star has a circumstellar disk and drives a ...
Investigation of the inner structures around HD169142 with VLT/SPHERE
(Oxford University Press, 2018)
We present observations of the Herbig Ae star HD 169142 with the VLT/SPHERE instruments InfraRed Dual-band Imager and Spectrograph (IRDIS) (K1K2 and H2H3 bands) and the Integral Field Spectrograph (IFS) (Y, J and H bands). ...
VLTI/PIONIER images the Achernar disk swell
(EDP Sciences, 2017-05)
Context. The mechanism of disk formation around fast-rotating Be stars is not well understood. In particular, it is not clear which mechanisms operate, in addition to fast rotation, to produce the observed variable ejection ...