A Magellan-IMACS-IFU Search for Dynamical Drivers of Nuclear Activity. I. Reduction Pipeline and Galaxy Catalog
Paul Westoby, Carole Mundell, Neil Nagar, Witold Maciejewski, Eric, Emsellem, Martin Roth, Joris Gerssen, Ivan Baldry

TL;DR
This study introduces a new reduction pipeline for IMACS-IFU data and presents galaxy kinematic maps, aiming to understand the dynamical triggers of nuclear activity in Seyfert and inactive galaxies.
Contribution
It provides the first detailed data reduction and calibration procedure for IMACS-IFU long mode observations and presents a comprehensive galaxy sample with kinematic maps.
Findings
First detailed IMACS-IFU data reduction pipeline
Galaxy kinematic maps and properties presented
Sample includes Seyfert and inactive control galaxies
Abstract
Using the Inamori Magellan Areal Camera and Spectrograph (IMACS) integral-field unit (IFU) on the 6.5m Magellan telescope, we have designed the first statistically significant investigation of the two-dimensional distribution and kinematics of ionized gas and stars in the central kiloparsec regions of a well-matched sample of Seyfert and inactive control galaxies selected from the Sloan Digital Sky Survey. The goals of the project are to use the fine spatial sampling (0.2 arcsec/pixel) and large wavelength coverage (4000-7000A) of the IMACS-IFU to search for dynamical triggers of nuclear activity in the central region where active galactic nucleus (AGN) activity and dynamical timescales become comparable, to identify and assess the impact of AGN-driven outflows on the host galaxy and to provide a definitive sample of local galaxy kinematics for comparison with future three-dimensional…
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