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Related papers: Resolving the dynamical mass of a z~1.3 QSO host g…

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We characterize the stellar mass of J2239+0207, a z~6.25 sub-Eddington quasar (M_1450=-24.6), using dedicated JWST/NIRCam medium-band observations of a nearby PSF star to remove the central point source and reveal the underlying galaxy…

Astrophysics of Galaxies · Physics 2023-08-07 Meredith Stone , Jianwei Lyu , George H. Rieke , Stacey Alberts

We investigate the relationship between the mass of the central supermassive black hole, M_bh, and the host galaxy luminosity, L_gal, in a sample of quasars from the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7). We use composite…

Astrophysics of Galaxies · Physics 2015-06-19 S. Salviander , G. A. Shields , E. W. Bonning

Correlations between the mass of a supermassive black hole and the properties of its host galaxy (e.g., total stellar mass (M*), luminosity (Lhost)) suggest an evolutionary connection. A powerful test of a co-evolution scenario is to…

At low redshift, there are fundamental correlations between the mass of supermassive black holes (MBH) and the mass (Mbulge) and luminosity of the host galaxy bulge. We investigate the same relation at z>=1. Using virial mass estimates for…

Astrophysics · Physics 2009-11-13 Chien Y. Peng , Chris D. Impey , Luis C. Ho , Elizabeth J. Barton , Hans-Walter Rix

ALMA [CII] line and continuum observations of five redshift z>6 quasars are presented. This sample was selected to probe lower black hole mass quasars than most previous studies. We find a wide dispersion in properties with CFHQS…

Astrophysics of Galaxies · Physics 2017-12-06 Chris J. Willott , Jacqueline Bergeron , Alain Omont

Recently, the relation between the masses of the black hole ($M_{BH}$) and the host galaxy ($M_{host}$) in quasars has been probed down to the parameter space of $M_{BH}\sim10^8 M_\odot$ and $M_{host}\sim10^{11} M_\odot$ at z $<$ 0.5. In…

Astrophysics of Galaxies · Physics 2014-10-14 Jimit Sanghvi , Jari Kotilainen , Renato Falomo , Roberto Decarli , Kalle Karhunen , Michela Uslenghi

We combine Hubble Space Telescope images from the Great Observatories Origins Deep Survey with archival Very Large Telescope and Keck spectra of a sample of 11 X-ray selected broad-line active galactic nuclei in the redshift range 1<z<2 to…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Vardha N. Bennert , Matthew W. Auger , Tommaso Treu , Jong-Hak Woo , Matthew A. Malkan

Our knowledge of relations between supermassive black holes and their host galaxies at $z\gtrsim1$ is still limited, even though being actively sought out to $z\sim6$. Here, we use the high resolution and sensitivity of JWST to measure the…

We measure the correlation between black-hole mass $M_{\rm BH}$ and host stellar mass $M_*$ for a sample of 38 broad-line quasars at $0.2\lesssim z\lesssim 0.8$ (median redshift $z_{\rm med}=0.5$). The black-hole masses are derived from a…

We present a dynamical analysis of a quasar-host galaxy at $z\simeq 6$ (SDSS J2310+1855) using a high-resolution ALMA observation of the [CII] emission line. The observed rotation curve was fitted with mass models that considered the…

In the present-day universe, supermassive black hole masses (MBH) appear to be strongly correlated with their galaxy's bulge luminosity, among other properties. In this study, we explore the analogous relationship between MBH, derived using…

We present and analyse the deepest, high-quality Ks-band images ever obtained of luminous quasars at z~4, in an attempt to determine the basic properties of their host galaxies less than 1 Gyr after the first recorded appearance of black…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Thomas A. Targett , James S. Dunlop , Ross J. McLure

In the local universe, the masses of Super-Massive Black-Holes (SMBH) appear to correlate with physical properties of their hosts, including the mass of the dark-matter halos. At higher redshifts, we observe the growth of SMBHs indirectly…

Astrophysics · Physics 2009-11-10 Stuart Wyithe , T. Padmanabhan

Quasars are useful tracers of the cosmological evolution of the black hole mass - galaxy relation. We compare the expectations of Semi-Analytical Models (SAM) of galaxy evolution, to the largest available datasets of quasar host galaxies…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 L. Portinari , J. Kotilainen , R. Falomo , R. Decarli

We measure host galaxy stellar masses for a sample of five luminous quasars at $z\sim5-7$. Using JWST/NIRCam medium-band images of nearby PSF reference stars, we carefully subtract the contribution from the quasar light to place upper and…

Astrophysics of Galaxies · Physics 2024-02-07 Meredith A. Stone , Jianwei Lyu , George H. Rieke , Stacey Alberts , Kevin N. Hainline

[Abridged] To investigate the evolution in the relation between galaxy stellar and central black hole mass we construct a volume limited complete sample of 85 AGN with host galaxy stellar masses M_{*} > 10^{10.5} M_{sol}, and specific X-ray…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Asa F. L. Bluck , Christopher J. Conselice , Omar Almaini , Elise S. Laird , Kirpal Nandra , Ruth Gruetzbauch

Understanding the relationship between the formation and evolution of galaxies and their central super massive black holes (SMBH) is one of the main topics in extragalactic astrophysics. Links and feedback may reciprocally affect both black…

Strongly lensed active galactic nuclei (AGN) provide a unique opportunity to make progress in the study of the evolution of the correlation between the mass of supermassive black holes ($\mathcal M_{BH}$) and their host galaxy luminosity…

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