The $M_{\mathrm{BH}}-M_{\star }$ Relation of the hyperluminous Dust-obscured Quasars up to $z\sim 4$

Abstract

Hot dust-obscured galaxies (Hot DOGs) are a rare population of hyperluminous dust-obscured quasars discovered by the Wide-field Infrared Survey Explorer (WISE) all-sky survey. The heavy circumnuclear dust obscuration allows only a small amount of scattered light from the obscured quasar to escape, enabling the decomposition of the stellar component from the total flux. The presence of scattered light enables the redshift of the source and the properties of the black hole to be obtained from SDSS and SDSS-related literature. From WISE and SDSS data, we select 11 hyperluminous Hot DOGs at $z=1.5-3.7$ with bolometric luminosities $L_{\mathrm{bol}}\gtrsim 10^{47}\mathrm{erg}{\mathrm{s}}^{-1}$. We investigate the $M_{\mathrm{BH}}-M_{\star }$ relation in these sources using Bayesian spectral energy distribution (SED) fitting or with extra constraints from \textit{Hubble Space Telescope} (HST) image decomposition. Stellar masses are successfully derived for eight Hot DOGs. We find high Eddington ratios ${\lambda }_{\mathrm{Edd}}$ in these Hot DOGs, with the median value of 1.05 and the maximum value close to 3. The super-Eddington accretion may be associated with the overdense environments of Hot DOGs. We find no significant differences in the $M_{\mathrm{BH}}/M_{\star }$ of these Hot DOGs compared to the local relation, suggesting that these dust-obscured quasars are the progenitors of massive early-type galaxies. We speculate that the subsequent evolution of Hot DOGs may be significantly influenced by AGN feedback and remain on the local relation.

arXiv comment14 pages, 5 figures, Accepted for pubulication in AAS journal

References in corpus (92)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• The Demography of Massive Dark Objects in Galaxy Centres
• Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy
• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• The Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions
• The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory
• The Herschel-SPIRE instrument and its in-flight performance
• On the Black Hole Mass - Bulge Mass Relation
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
• CIGALE: a python Code Investigating GALaxy Emission
• Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
• AGN Dusty Tori: II. Observational Implications of Clumpiness
• The Pan-STARRS1 Database and Data Products
• AGN Dusty Tori: I. Handling of Clumpy Media
• What Drives the Growth of Black Holes?
• The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
• Obscured Active Galactic Nuclei
• On the cosmic evolution of the scaling relations between black holes and their host galaxies: Broad Line AGN in the zCOSMOS survey
• The Dark Energy Survey Data Release 2
• X-CIGALE: fitting AGN/galaxy SEDs from X-ray to infrared
• The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V
• Molecular Gas in Redshift 6 Quasar Host Galaxies
• The First Hyper-Luminous Infrared Galaxy Discovered by WISE
• The mass relations between supermassive black holes and their host galaxies at 1<z<2 with HST-WFC3
• Massive Galaxies in COSMOS: Evolution of Black hole versus bulge mass but not versus total stellar mass over the last 9 Gyrs?
• Half of the Most Luminous Quasars May Be Obscured: Investigating the Nature of WISE-Selected Hot, Dust-Obscured Galaxies
• The Relationship Between Stellar and Black-Hole Mass in Submillimeter Galaxies
• Weighing the Black Holes in z~2 Submillimeter-Emitting Galaxies Hosting Active Galactic Nuclei
• A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16
• Cosmic Evolution of Black Holes and Spheroids. III. The M-sigma relation in the last six billion years
• Cosmic Evolution of Black Holes and Spheroids. II: Scaling Relations at z=0.36
• The Most Luminous Galaxies Discovered by WISE
• Submillimeter Follow-up of WISE-Selected Hyperluminous Galaxies
• The UKIRT Hemisphere Survey: Definition and J-band Data Release
• The VVDS type-1 AGN sample: The faint end of the luminosity function
• No significant evolution of relations between Black hole mass and Galaxy total stellar mass up to z~2.5
• Detection of stellar light from quasar host galaxies at redshifts above 6
• NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-Selected Quasars at z ~ 2
• The black hole - bulge mass relation of Active Galactic Nuclei in the Extended Chandra Deep Field - South Survey
• A Local Baseline of the Black Hole Mass Scaling Relations for Active Galaxies. I. Methodology and Results of Pilot Study
• The most-luminous heavily-obscured quasars have a high merger fraction: morphological study of WISE-selected hot dust-obscured galaxies
• On the difference of torus geometry between hidden and non-hidden broad line active galactic nuclei
• EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\gtrsim 6$
• The M_BH - M_star relation for X-ray obscured, red QSOs at 1.2< z <2.6
• Spitzer Observations of Young Red Quasars
• The WISSH quasars Project: II. Giant star nurseries in hyper-luminous quasars
• The primordial environment of super massive black holes: large scale galaxy overdensities around $z\sim 6$ QSOs with LBT
• The Strikingly Uniform, Highly Turbulent Interstellar Medium of the Most Luminous Galaxy in the Universe
• Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxies
• ALMA detections of CO emission in the most luminous, heavily dust-obscured quasars at z>3
• Hot Dust Obscured Galaxies with Excess Blue Light: Dual AGN or Single AGN Under Extreme Conditions?
• Multi-wavelength properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
• The Multiple Merger Assembly of a Hyper-luminous Obscured Quasar at redshift 4.6
• Heavy X-ray obscuration in the most-luminous galaxies discovered by WISE
• Evolutionary Paths of Active Galactic Nuclei and Their Host Galaxies
• Infrared spectral energy distribution decomposition of WISE-selected, hyperluminous hot dust-obscured galaxies
• Eddington-Limited Accretion in z~2 WISE-selected Hot, Dust-Obscured Galaxies
• Cosmic Evolution of Black Holes and Spheroids. V. The Relation Between Black Hole Mass and Host Galaxy Luminosity for a Sample of 79 Active Galaxies
• The Sizes of Quasar Host Galaxies with the Hyper Suprime-Cam Subaru Strategic Program
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• Host galaxies of high-redshift extremely red and obscured quasars
• The hidden quasar nucleus of a WISE-selected, hyperluminous, dust-obscured galaxy at z ~ 2.3
• Synchronized Co-evolution between Supermassive Black Holes and Galaxies Over the Last Seven Billion Years as Revealed by the Hyper Suprime-Cam
• Hot Dust-Obscured Galaxies with Excess Blue Light
• Decoding spectral energy distributions of dust-obscured starburst-AGN
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• Super-Eddington Accretion in the WISE-Selected Extremely Luminous Infrared Galaxy W2246-0526
• Fast Outflows in Hot Dust-Obscured Galaxies with Keck/NIRES
• A quasar-galaxy merger at $z\sim 6.2$: black hole mass and quasar properties from the NIRSpec spectrum
• Spectral Classification and Ionized Gas Outflows in $z\sim 2$ WISE-Selected Hot Dust-Obscured Galaxies
• The Sloan Digital Sky Survey Reverberation Mapping Project: The M_BH-Host Relations at 0.2<z<0.6 from Reverberation Mapping and Hubble Space Telescope Imaging
• The M_BH-M_star relation of obscured AGNs at high redshift
• A quasar-galaxy merger at $z\sim 6.2$: rapid host growth via accretion of two massive satellite galaxies
• Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913
• Imaging Polarization of the Blue-Excess Hot Dust-Obscured Galaxy WISE J011601.41-050504.0
• No evidence for a significant evolution of $M_{\bullet }$-$M_{\ast }$ relation in massive galaxies up to z$\sim$4
• Black Hole Masses and Star Formation Rates of z >1 Dust Obscured Galaxies (DOGs): Results from Keck OSIRIS Integral Field Spectroscopy
• Testing the Evolution of the Correlations between Supermassive Black Holes and their Host Galaxies using Eight Strongly Lensed Quasars
• The spectral energy distribution of the hyperluminous, hot dust-obscured galaxy W2246$-$0526
• SOFIA/HAWC+ View of an Extremely Luminous Infrared Galaxy, WISE1013+6112
• An Overdensity of Lyman Break Galaxies Around the Hot Dust-Obscured Galaxy WISE J224607.56$-$052634.9
• An overdensity of red galaxies around the hyperluminous dust-obscured quasar W1835$+$4355 at $z=2.3$
• Physical properties of hyperluminous, dust-obscured quasars at $z\sim 3$: multiwavelength Spectral Energy Distribution analysis and cold gas content revealed by ALMA
• An extreme EXO: a type 2 QSO at z=1.87
• Discovery of a Low-Redshift Hot Dust-Obscured Galaxy
• A new approach to constraining properties of AGN host galaxies by combining image and SED decomposition: testing upon the MBH-M* relation
• Searching for Low-Redshift Hot Dust-Obscured Galaxies

Cited by in corpus (2)

• ALMA High-J CO Spectroscopy of High-Redshift Galaxies. II. 0.03" Resolution CO Kinematics Reveal Super-Eddington Accretion in a Dust-Obscured Galaxy at z=3.111
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth