activity
19992026
most citedA diversity of dusty AGN tori: Data release for the VLTI/MIDI AGN Large Program and first results for 23 galaxies

256 citations · 3.6k across the 72 of their papers we have counts for

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18 papers · 1 filter

astro-ph2008★ 38 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★ 4 cited

AGN accretion disks as spatially resolved by polarimetry

Makoto Kishimoto, Robert Antonucci, Omer Blaes +4

A crucial difficulty in understanding the nature of the putative accretion disk in AGNs is that some of its key intrinsic spectral signatures cannot be observed directly. The stron…

astro-ph2008★ 146 cited

The characteristic blue spectra of accretion disks in quasars as uncovered in the infrared

Makoto Kishimoto, Robert Antonucci, Omer Blaes +4

Quasars are thought to be powered by supermassive black holes accreting surrounding gas. Central to this picture is a putative accretion disk which is believed to be the source of…

astro-ph2008★ 20 cited

Discovery of a strong Baldwin effect in mid-infrared AGN lines

S. F. Hoenig, A. Smette, T. Beckert +5

We present the discovery of a Baldwin effect in 8 nearby Seyfert galaxies for the three most prominent mid-infrared forbidden emission lines observable from the ground that are com…

astro-ph2007★ 220 cited

The innermost region of AGN tori: implications from the HST/NICMOS Type 1 point sources and near-IR reverberation

Makoto Kishimoto, Sebastian F. Hoenig, Thomas Beckert +1

Spatially resolving the innermost torus in AGN is one of the main goals of its high-spatial-resolution studies. This could be done in the near-IR observations of Type 1 AGNs where…

astro-ph2006

Resolving the BLR in NGC 3783

P. Lira, M. Kishimoto, A. Robinson +5

We present results from very high signal-to-noise spectropolarimetric observations of the Seyfert 1 galaxy NGC 3783. Position Angle (PA) changes across the Balmer lines show that t…