PI: Fred Hamann, U. of Florida, email@example.com
Address: Department of Astronomy, PO Box 112055, 211 Bryant Space Science Center, Gainesville, FL, 32611-2055 USA
CoI: Nadia Zakamska, Johns Hopkins U.
CoI: Rachael Alexandroff, Johns Hopkins U.
CoI: Kelly Denny, Ohio State U.
CoI: Guilin Liu, Johns Hopkins U.
CoI: Isabelle Paris, Osservatorio Astronomico di Trieste
CoI: Nicholas Ross, University of Edinburgh
Title: Outflows & Feedback in Extremely Red Quasars
Abstract: Red quasars are candidate young objects participating in the early stages of massive galaxy formation. We recently completed a survey that finds ~200 high-redshift extremely red quasars (ERQs) in SDSS- III/BOSS based on rest-frame UV-MIR colors. These unique sources characteristically have extreme emission line properties that appear to result from extended outflowing emitting regions. We confirmed the connection to powerful outflows for 4 ERQs where VLT/XSHOOTER spectra reveal the broadest and most blueshifted [OIII] lines ever reported (with FHMMs and blueshifted wings reaching 5000km/s). These are large-scale outflows that might drive feedback to the host galaxies. We now propose GNIRS observations of 10 more ERQs to test the ubiquity of [OIII] outflows in the ERQ population, study the nature and origins of these outflows, and estimate their kinetic energies compared to models of feedback in galaxy evolution.
Program Type: Standard/Extragalactic
Run 1 (2016A): GEM-NQ/GNIRS -- 30hrs band 3 (GN-2016A-Q-90)
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360