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Andrew Robinson

Researcher at Rochester Institute of Technology

Publications -  94
Citations -  2846

Andrew Robinson is an academic researcher from Rochester Institute of Technology. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 29, co-authored 93 publications receiving 2655 citations. Previous affiliations of Andrew Robinson include University of Hertfordshire & Netherlands Institute for Space Research.

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Spitzer irs spectra of a large sample of seyfert galaxies: a variety of infrared spectral energy distributions in the local active galactic nucleus population

TL;DR: In this article, the results of a large-scale Spitzer IRS low-resolution spectroscopy of a statistically representative subsample of 51 of the Seyfert galaxies (59%) were presented, with an analysis of the continuum shapes and spectral features.
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Spitzer IRS spectra of a large sample of Seyfert galaxies: a variety of infrared SEDs in the local AGN population

TL;DR: In this paper, the results of IRS low-resolution spectroscopy of a statistically representative subsample of 51 of the galaxies (59%) were presented, with an analysis of the continuum shapes and a comparison of the Seyfert types.
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Streaming Motions Towards the Supermassive Black Hole in NGC 1097

TL;DR: In this paper, the authors used GMOS-IFU and high resolution HST-ACS observations to map the gas velocity field and structure within the 0.7 kpc circumnuclear ring of the SBb LINER/Seyfert 1 galaxy NGC 1097.
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Streaming Motions toward the Supermassive Black Hole in NGC 1097

TL;DR: In this paper, the authors used GMOS-IFU and high-resolution HST-ACS observations to map the gas velocity field and structure within the 0.7 kpc circumnuclear ring of the SBb LINER/Seyfert 1 galaxy NGC 1097.
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Nuclear Spirals as Feeding Channels to the Supermassive Black Hole: The Case of the Galaxy NGC 6951

TL;DR: In this article, the authors reported the discovery of gas streaming motions along nuclear spiral arms toward the LINER nucleus of the galaxy NGC 6951, which supports a scenario in which nuclear spirals are channels through which matter is transferred from galactic scales to the nuclear region to feed the supermassive black hole.