ACTIVE GALACTIC NUCLEUS HOST GALAXY MORPHOLOGIES IN COSMOS

By J. Gabor, C. Impey, K. Jahnke, B. Simmons, J. Trump, A. Koekemoer, M. Brusa, N. Cappelluti, E. Schinnerer, V. Smolčić and 7 more. 2009

167 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/363812442e51c14ae56eefb441d467f47a96d9f9

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Citations in the corpus

Cosmic X-ray surveys of distant active galaxies (2015, background): “…to reside in a broad range of host-galaxy types out to at least z ≈ 3, from disk-dominated to bulge-dominated systems (e.g., Grogin et al 2005; Pierce et al 2007, 2010b; Gabor et al 2009; Georgakakis et al 2009; Cisternas et al 2011, 2014; Kocevski et al 2012; Böhm et al 2013; Fan et al 2014).”
The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe (2014, result): “…results are consistent with most other investigations of the less powerful AGN population over the same range in redshift (e.g. Pierce et al. 2007, Gabor et al. 2009, Hickox et al. 2009, Silverman et al. 2009, 2011, Schawinski et al. 2011, Kocevski et al. 2012, Mullaney et al. 2012a,b, Aird et…”
THE XMM-NEWTON WIDE-FIELD SURVEY IN THE COSMOS FIELD (XMM-COSMOS): DEMOGRAPHY AND MULTIWAVELENGTH PROPERTIES OF OBSCURED AND UNOBSCURED LUMINOUS ACTIVE GALACTIC NUCLEI (2010, background): “…confirmed AGN (Gilli et al. 2009); the space density of high-redshift QSOs (Brusa et al. 2009); the host galaxies properties of AGN in COSMOS (Gabor et al. 2009); the on-going and co-evolving starformation and AGN activity at z< 0.8 (Silverman et al. 2009a); the environments of AGN within…”
THE BULK OF THE BLACK HOLE GROWTH SINCE z ∼ 1 OCCURS IN A SECULAR UNIVERSE: NO MAJOR MERGER–AGN CONNECTION (2010, methodology): “Our results agree with the few recent studies that have used a control sample (Dunlop et al. 2003; Grogin et al. 2003, 2005; Pierce et al. 2007; Gabor et al. 2009; Reichard et al. 2009; Tal et al. 2009, and also with recent results from the E-CDFS by Böhm et al. 2010, submitted), in the sense that…”
Morphologies of z ∼ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity (2014, background): “…when host galaxies of AGN are compared to galaxies of similar mass they show comparable incidences of disturbances indicative of recent mergers (Dunlop et al. 2003; Grogin et al. 2005; Pierce et al. 2007, 2010; Gabor et al. 2009; Cisternas et al. 2011; Kocevski et al. 2012; Boehm et al. 2013).”
Galaxy pairs in the Sloan Digital Sky Survey - IV: Interactions trigger AGN (2011, background): “…sole AGN trigger (e.g. Li et al. 2006; Lutz et al. 2010; Mullaney et al. 2011), which may play a role in explaining why many imaging surveys of AGN hosts detect no signs of (an excess of) recent merger activity (e.g. Grogin et al. 2005; Gabor et al.2009; Cisternas et al 2011; Kocevski et al. 2011).”
BLACK HOLE GROWTH AND ACTIVE GALACTIC NUCLEI OBSCURATION BY INSTABILITY-DRIVEN INFLOWS IN HIGH-REDSHIFT DISK GALAXIES FED BY COLD STREAMS (2011, background): “Host galaxies of moderate-luminosity AGNs do not show an excess of majormerger signatures (Grogin et al. 2005; Gabor et al. 2009) and often have disky morphologies (Schawinski et al. 2011).”
The Evolution of Galaxy Structure Over Cosmic Time (2014, background): “However, studies at higher redshifts generally do not find that more asymmetric or merging galaxies have a higher AGN fraction (e.g., Grogin et al. 2005; Gabor et al. 2009; Kocevski et al. 2012).”
Galaxy Interactions Trigger Rapid Black Hole Growth: an unprecedented view from the Hyper Suprime-Cam Survey (2017, result): “Previous studies that have investigated merger–AGN connections have produced mixed results (e.g. Gabor et al. 2009; Cisternas et al. 2011; Schawinski et al. 2011; Kocevski et al. 2012; Treister et al. 2012; Ellison et al. 2013; Villforth et al. 2014; Kocevski et al. 2015), often finding that the…”
RELATIONS BETWEEN CENTRAL BLACK HOLE MASS AND TOTAL GALAXY STELLAR MASS IN THE LOCAL UNIVERSE (2015, result): “We find that a significant fraction of local broadline AGN host galaxies are also spirals/disks, similar to what has previously been found in studies of moderate-luminosity AGN host galaxies out to z ∼ 3 (e.g., Gabor et al. 2009; Schawinski et al. 2011; Kocevski et al. 2012; Bennert et al. 2015).”
CANDELS: CONSTRAINING THE AGN–MERGER CONNECTION WITH HOST MORPHOLOGIES AT z ∼ 2 (2011, background): “More recently, Gabor et al. (2009) and Cisternas et al. (2011) examined the host morphologies of AGNs selected in the Cosmic Evolution Survey (COSMOS; Scoville et al. 2007) and report that the disturbed fraction among active and quiescent galaxies at z ∼ 1 is not significantly different.”
Growth and activity of black holes in galaxy mergers with varying mass ratios (2014, unknown): “…of ∼400 AGN hosts and of a control sample of inactive galaxies from the Cosmic Evolution Survey (COSMOS) field at redshifts 0.3 < z < 1.0, c© 0000 RAS Gabor et al. (2009) find that the asymmetry distributions and the neighbour counts of the two samples are consistent with each other, suggesting…”
Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations (2012, background): “2005; Gabor et al. 2009; Cisternas et al. 2011), and are frequently found in disks at high redshifts (Schawinski et al. 2011; Kocevski et al. 2012).”
CONSTRAINTS ON BLACK HOLE GROWTH, QUASAR LIFETIMES, AND EDDINGTON RATIO DISTRIBUTIONS FROM THE SDSS BROAD-LINE QUASAR BLACK HOLE MASS FUNCTION (2010, background): “Indeed, many AGNs are observed to live in late-type galaxies out to z ≈ 1 (e.g., Guyon et al. 2006; Gabor et al. 2009), and the X-ray luminosity function of AGNs hosted by late-type galaxies suggests that fueling by minor interactions or internal instabilities represents a non-negligible…”
Galaxy pairs in the Sloan Digital Sky Survey – IX. Merger-induced AGN activity as traced by the Wide-field Infrared Survey Explorer (2014, background): “…studies that have looked for an excess of tidal features or distorted morphologies in AGN versus nonAGN galaxies, have found no statistical difference both at low (e.g., Gabor et al. 2009; Reichard et al. 2009; Cisternas et al. 2011; Kocevski et al. 2011; Bohm et al. 2012), intermediate(0.5”
THE CHANDRA COSMOS SURVEY. III. OPTICAL AND INFRARED IDENTIFICATION OF X-RAY POINT SOURCES (2012, background): “…not to be contaminated by unobscured AGN, for which the presence of a bright nuclear source can affect the determination of the concentration index (Gabor et al. 2009), we excluded from the sample sources classified as point-like from the ACS catalog (Leauthaud et al. 2007) and also sources…”
MID-INFRARED SELECTION OF ACTIVE GALACTIC NUCLEI WITH THE WIDE-FIELD INFRARED SURVEY EXPLORER. I. CHARACTERIZING WISE-SELECTED ACTIVE GALACTIC NUCLEI IN COSMOS (2012, background): “Griffith & Stern (2010) have recently analyzed the optical morphologies of AGN in the COS- MOS field identified from a variety of methods: radio selection, X-ray selection, and mid-infrared selection (see also Gabor et al. 2009).”
What drives the growth of black holes (2011, background): “…AGNs are also comparable to those of similarly massive inactive galaxies (e.g., Sánchez et al., 2004; Grogin et al., 2005; Pierce et al., 2007; Gabor et al., 2009; Georgakakis et al., 2009; Kocevski et al., 2011; Schawinski et al., 2011), with a mix of bulge-dominated and discdominated…”