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M. Kishimoto

72 papers hereh-index 272.9k citations110 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author16
  • middle author33
  • last author8

Across the 58 of 72 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA33
  • astro-ph18
  • astro-ph.CO14
  • astro-ph.IM4
  • astro-ph.SR2
  • astro-ph.HE1
same name
  • M. Kishimoto — 1 paper, h 19
  • M. Kishimoto — 1 paper, h 18

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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

collaborators
Showing 2017 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2017★ 35 cited

A mid-infrared statistical investigation of clumpy torus model predictions

J. García-González, A. Alonso-Herrero, S. F. Hönig +7

We present new calculations of the CAT3D clumpy torus models, which now include a more physical dust sublimation model as well as AGN anisotropic emission. These new models allow g…

astro-ph.GA2017★ 70 cited

PAH features within few hundred parsecs of active galactic nuclei

J. J. Jensen, S. F. Hönig, S. Rakshit +6

Spectral features from PAH molecules observed in the mid-IR range are typically used to infer the amount of recent and ongoing star formation (SF) on kpc scales around AGN where mo…

astro-ph.GA2017★ 172 cited

Dusty winds in active galactic nuclei: reconciling observations with models

Sebastian F. Hönig, Makoto Kishimoto

This letter presents a revised radiative transfer model for the infrared (IR) emission of active galactic nuclei (AGN). While current models assume that the IR is emitted from a du…

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