activity
19942006
most citedVLTI/VINCI observations of the nucleus of NGC 1068 using the adaptive optics system MACAO

65 citations · 73 across the 5 of their papers we have counts for

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40 papers · 1 filter

astro-ph200838 cited

Possible evidence for a common radial structure in nearby AGN tori

Makoto Kishimoto, Sebastian F. Hoenig, Konrad R. W. Tristram +1

We present a quantitative and relatively model-independent way to assess the radial structure of nearby AGN tori. These putative tori have been studied with long-baseline infrared…

astro-ph2008

Phase Closure Image Reconstruction for Future VLTI Instrumentation

Mercedes E. Filho, Stephanie Renard, Paulo Garcia +21

Classically, optical and near-infrared interferometry have relied on closure phase techniques to produce images. Such techniques allow us to achieve modest dynamic ranges. In order…

astro-ph2008

Phase Referencing in Optical Interferometry

Mercedes E. Filho, Paulo Garcia, Gilles Duvert +20

One of the aims of next generation optical interferometric instrumentation is to be able to make use of information contained in the visibility phase to construct high dynamic rang…

astro-ph2008

System overview of the VLTI Spectro-Imager

L. Jocou, J. P. Berger, F. Malbet +30

The VLTI Spectro Imager project aims to perform imaging with a temporal resolution of 1 night and with a maximum angular resolution of 1 milliarcsecond, making best use of the Very…

astro-ph200826 cited

Asymmetric silicate dust distribution toward the silicate carbon star BM Gem

Keiichi Ohnaka, Hideyuki Izumiura, Christoph Leinert +3

Silicate carbon stars show the 10 micron silicate emission, despite their carbon-rich photospheres. They are considered to have circumbinary or circum-companion disks, which serve…

astro-ph2008157 cited

The origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry

S. Kraus, K. -H. Hofmann, M. Benisty +14

To trace the accretion and outflow processes around YSOs, diagnostic spectral lines such as the BrG 2.166 micron line are widely used, although due to a lack of spatial resolution,…