Gemini Imaging of the Host Galaxies of Changing-Look Quasars
arXiv:1903.08122 · doi:10.3847/1538-4357/ab0ec1
Abstract
Changing-look quasars are a newly-discovered class of luminous active galactic nuclei that undergo rapid (10 year) transitions between Type 1 and Type 1.9/2, with an associated change in their continuum emission. We characterize the host galaxies of four faded changing-look quasars using broadband optical imaging. We use \textit{gri} images obtained with the Gemini Multi Object Spectrograph (GMOS) on Gemini North to characterize the surface brightness profiles of the quasar hosts and search for [O III] emission from spatially extended regions, or voorwerpjes, with the goal of using them to examine past luminosity history. Although we do not detect, voorwerpjes surrounding the four quasar host galaxies, we take advantage of the dim nuclear emission to characterize the colors and morphologies of the host galaxies. Three of the four galaxies show morphological evidence of merger activity or tidal features in their residuals. The three galaxies which are not highly distorted are fit with a single Sérsic profile to characterize their overall surface brightness profiles. The single-Sérsic fits give intermediate Sérsic indices between the of disk galaxies and the of ellipticals. On a color-magnitude diagram, our changing-look quasar host galaxies reside in the blue cloud, with other AGN host galaxies and star-forming galaxies. On a color-Sérsic index diagram the changing-look quasar hosts reside with other AGN hosts in the "green valley". Our analysis suggests that the hosts of changing-look quasars are predominantly disrupted or merging galaxies that resemble AGN hosts, rather than inactive galaxies.
20 pages, 5 figures
References in corpus (16)
- The Host Galaxies and Classification of Active Galactic Nuclei
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk
- The Discovery of the First "Changing Look" Quasar: New Insights into the Physics & Phenomenology of AGN
- The Evolution of AGN Host Galaxies: From Blue to Red and the Influence of Large-Scale Structures
- iPTF Discovery of the Rapid "Turn On" of a Luminous Quasar
- The Close AGN Reference Survey (CARS) - Mrk 1018 returns to the shadows after 30 years as a Seyfert 1
- Galaxy And Mass Assembly (GAMA): the wavelength-dependent sizes and profiles of galaxies revealed by MegaMorph
- Extended Emission-Line Regions: Remnants of Quasar Superwinds?
- Fading AGN Candidates: AGN Histories and Outflow Signatures
- HST Imaging of Fading AGN Candidates I: Host-Galaxy Properties and Origin of the Extended Gas
- The Sudden Death of the Nearest Quasar
- Gemini Long-slit Observations of Luminous Obscured Quasars: Further Evidence for an Upper Limit on the Size of the Narrow-Line Region
- The Close AGN Reference Survey (CARS): Mrk 1018 halts dimming and experiences strong short-term variability
- Spatially-Resolved Spectra of the "Teacup" AGN: Tracing the History of a Dying Quasar
- An Active Galactic Nucleus Caught in the Act of Turning Off and On
Cited by in corpus (7)
- The Time Domain Spectroscopic Survey: Changing-Look Quasar Candidates from Multi-Epoch Spectroscopy in SDSS-IV
- A Systematic Analysis of Stellar Populations in the Host Galaxies of Changing-look AGNs
- Local Active Galactic Nuclei with Large Broad-Hα Variability Reside in Red Galaxies
- Host Galaxy Properties of Changing-look AGN Revealed in the MaNGA Survey
- Active galactic nuclei catalog from the AKARI NEP Wide field
- Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
- Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility