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astro-ph2001★ 81 cited
3--4 m Spectroscopy of Seyfert 2 Nuclei to Quantitatively Assess the Energetic Importance of Compact Nuclear Starbursts
Masatoshi Imanishi
We report on 3--4 m slit spectroscopy of 13 Seyfert 2 nuclei. The 3.3 m polycyclic aromatic hydrocarbon (PAH) emission is used to estimate the magnitudes of compact ( a fe…
astro-ph2001★ 49 cited
Strong Evidence for a Buried AGN in UGC 5101: Implications for LINER-Type Ultra-Luminous Infrared Galaxies
Masatoshi Imanishi, C. C. Dudley, Philip R. Maloney
We report on the results of 3--4 m spectroscopy of the ultra-luminous infrared galaxy (ULIRG) UGC 5101. It has a cool far-infrared color and a LINER-type optical spectrum, and s…
astro-ph2001★ 12 cited
Thermal Infrared 3--5 m Colors of Obscured and Unobscured Active Galactic Nuclei
Masatoshi Imanishi
Thermal infrared photometry in the - and -band and colors of type-1 and type-2 active galactic nuclei (AGNs) are presented. After combining our observations with ph…