H1821+643: The most X-ray and infrared luminous AGN in the Swift/BAT survey in the process of rapid stellar and supermassive black hole mass assembly

Abstract

H1821+643 is the most X-ray luminous non-beamed AGN of $L_{14-150keV}=5.2\times 10^{45}$ erg s${}^{-1}$ in the Swift/BAT ultra-hard X-ray survey and it is also a hyper-luminous infrared (IR) galaxy $L_{\mathrm{IR}}=10^{13.2}{L}_{\odot }$ residing in the center of a massive galaxy cluster, which is a unique environment achieving the rapid mass assembly of black holes (BH) and host galaxies in the local universe. We decompose the X-ray to IR spectral energy distribution (SED) into the AGN and starburst component using the SED fitting tool CIGALE-2022.0 and show that H1821+643 consumes a large amount of cold gas (${\dot{M}}_{\mathrm{con}}$) with star-formation rate of $\log (\mathrm{SFR}/M_{\odot }{\mathrm{yr}}^{-1})=3.01\pm 0.04$ and BH accretion rate of $\log ({\dot{M}}_{\mathrm{BH}}/M_{\odot }{\mathrm{yr}}^{-1})=1.20\pm 0.05$. This high ${\dot{M}}_{\mathrm{con}}$ is larger than the cooling rate (${\dot{M}}_{\mathrm{cool}}$) of the intra-cluster medium (ICM), ${\dot{M}}_{\mathrm{con}}/{\dot{M}}_{\mathrm{cool}}\gtrsim 1$, which is one to two order magnitude higher than the typical value of other systems, indicating that H1821 provides the unique and extreme environment of rapid gas consumption. We also show that H1821+643 has an efficient cooling path achieving from $10^7$ K to $10^2$ K thanks to [OIII] 63 $\mu \mathrm{m}$, which is a main coolant in low temperature range ($10^4$ K to $10^2$ K) with a cooling rate of ${\dot{M}}_{\mathrm{cool}}=3.2\times 10^5{M}_{\odot }\mathrm{y}{\mathrm{r}}^{-1}$, and the star-forming region extends over 40 kpc scale.

arXiv comment20 pages, 8 figures, accepted for publication in ApJ

References in corpus (124)

• Stellar population synthesis at the resolution of 2003
• The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
• Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• The Global Schmidt Law in Star Forming Galaxies
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• Energy input from quasars regulates the growth and activity of black holes and their host galaxies
• Correcting for the Effects of Interstellar Extinction
• Observational Evidence of AGN Feedback
• The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
• Advection-Dominated Accretion: A Self-Similar Solution
• The Star Formation Efficiency in Nearby Galaxies: Measuring Where Gas Forms Stars Effectively
• The Infrared Spectrograph on the Spitzer Space Telescope
• A Catalog of Quasar Properties from SDSS DR7
• Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies
• Towards a unified model for black hole X-ray binary jets
• CIGALE: a python Code Investigating GALaxy Emission
• Nuclear Activity in Nearby Galaxies
• GOODS-Herschel: an infrared main sequence for star-forming galaxies
• Cool Gas in High Redshift Galaxies
• Observational constraints on growth of massive black holes
• A Systematic Study of Radio-Induced X-ray Cavities in Clusters, Groups, and Galaxies
• The Molecular Interstellar Medium in Ultraluminous Infrared Galaxies
• Radiation Pressure Supported Starburst Disks and AGN Fueling
• Advection-Dominated Accretion: Self-Similarity and Bipolar Outflows
• The Assembly of the First Massive Black Holes
• The 70 Month Swift-BAT All-Sky Hard X-Ray Survey
• Determining Star Formation Rates for Infrared Galaxies
• Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
• X-ray emission from star-forming galaxies - I. High-mass X-ray binaries
• BAT AGN Spectroscopic Survey - V. X-ray properties of the Swift/BAT 70-month AGN catalog
• A Molecular Star Formation Law in the Atomic Gas Dominated Regime in Nearby Galaxies
• High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies
• How Do Massive Black Holes Get Their Gas?
• Piecing Together the X-ray Background: Bolometric Corrections for Active Galactic Nuclei
• Advection-Dominated Accretion and the Black Hole Event Horizon
• What is a Cool-Core Cluster? A Detailed Analysis of the Cores of the X-ray Flux-Limited HIFLUGCS Cluster Sample
• The dust covering factor in active galactic nuclei
• Bolometric luminosities and Eddington ratios of X-ray selected Active Galactic Nuclei in the XMM-COSMOS survey
• The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky Survey
• The 105 month Swift-BAT all-sky hard X-ray survey
• The Infrared Camera (IRC) for AKARI - Design and Imaging Performance
• Three-dimensional radiative transfer modeling of AGN dusty tori as a clumpy two-phase medium
• A Two-Parameter Model for the Infrared/Submillimeter/Radio Spectral Energy Distributions of Galaxies and AGN
• Diagnostics of irradiated dense gas in galaxy nuclei. II. A grid of XDR and PDR models
• Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies
• Photometric redshift and classification for the XMM-COSMOS sources
• Resolving the mid-infrared cores of local Seyferts
• BAT AGN Spectroscopic Survey I: Spectral Measurements, Derived Quantities, and AGN Demographics
• Compton-thick Accretion in the local Universe
• Black hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231
• CASSIS: The Cornell Atlas of Spitzer/IRS Sources
• The Far-Infrared Surveyor (FIS) for AKARI
• The Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z=2.5: Results from PEP-Herschel
• Galaxy Zoo : 'Hanny's Voorwerp', a quasar light echo?
• X-CIGALE: fitting AGN/galaxy SEDs from X-ray to infrared
• Dust Reddening in SDSS Quasars
• A diversity of dusty AGN tori: Data release for the VLTI/MIDI AGN Large Program and first results for 23 galaxies
• Accreting SMBHs in the COSMOS field and the connection to their host galaxies
• Investigating AGN Heating in a Sample of Nearby Clusters
• Constraining the properties of AGN host galaxies with Spectral Energy Distribution modeling
• A dominant population of optically invisible massive galaxies in the early Universe
• A Compendium of Far-Infrared Line and Continuum Emission for 227 Galaxies Observed by the Infrared Space Observatory
• Black Hole Growth to z = 2 - I: Improved Virial Methods for Measuring M_BH and L/L_Edd
• Dust in the polar region as a major contributor to the IR emission of AGN
• Fitting AGN/galaxy X-ray-to-radio SEDs with CIGALE and improvement of the code
• The subarcsecond mid-infrared view of local active galactic nuclei: I. The N- and Q-band imaging atlas
• The distribution of silicate strength in Spitzer spectra of AGNs and ULIRGs
• Radiative efficiency, variability and Bondi accretion onto massive black holes: from mechanical to quasar feedback in brightest cluster galaxies
• Star formation relations and CO SLEDs across the J-ladder and redshift
• The Relationship Between Black Hole Growth and Star Formation in Seyfert Galaxies
• Parsec-scale dust emission from the polar region in the type 2 nucleus of NGC 424
• Main sequence of star forming galaxies beyond the Herschel confusion limit
• The host galaxies of luminous quasars
• A 17-billion-solar-mass black hole in a group galaxy with a diffuse core
• Redefining the torus: A unifying view of AGN in the infrared and sub-mm
• Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies
• Normal, Dust-Obscured Galaxies in the Epoch of Reionization
• Molecular gas and star formation in early-type galaxies
• A Debris Disk around the Central Star of the Helix Nebula?
• The optically-powerful quasar E1821+643 is associated with a 300-kpc scale FRI radio structure
• The Complete Infrared View of Active Galactic Nuclei from the 70-month Swift/BAT Catalog
• BAT AGN Spectroscopic Survey - XI. The Covering Factor of Dust and Gas in Swift/BAT Active Galactic Nuclei
• CASSIS: The Cornell Atlas of Spitzer/Infrared Spectrograph Sources. II. High-resolution observations
• ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster
• BAT AGN Spectroscopic Survey - IV: Near-Infrared Coronal Lines, Hidden Broad Lines, and Correlation with Hard X-ray Emission
• Mid and Far Infrared Properties of a Complete Sample of Local AGNs
• Dissecting the active galactic nucleus in Circinus -- II. A thin dusty disc and a polar outflow on parsec scales
• The largest black holes and the most luminous galaxies
• Far-infrared line spectra of active galaxies from the Herschel/PACS Spectrometer: the complete database
• Sub-millimetre observations of hyperluminous infrared galaxies
• Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales
• SHINING, A Survey of Far Infrared Lines in Nearby Galaxies. I: Survey Description, Observational Trends, and Line Diagnostics
• Polar Dust, Nuclear Obscuration and IR SED Diversity in Type-1 AGNs
• Rest-frame Optical Spectra and Black Hole Masses of 3<z<6 Quasars
• NuSTAR observations of WISE J1036+0449, a Galaxy at z$\sim 1$ obscured by hot dust
• The X-ray luminous cluster underlying the bright radio-quiet quasar H1821+643
• The Swift/BAT AGN Spectroscopic Survey -- IX. The Clustering Environments of an Unbiased Sample of Local AGN
• The Most Massive Active Black-Holes at z~1.5-3.5 Have High Spins and Radiative Efficiencies
• Herschel-PACS spectroscopy of IR-bright galaxies at high redshift
• Is there a maximum mass for black holes in galactic nuclei?
• The first measurement of the quasar lifetime distribution
• The Rarity of Star Formation in Brightest Cluster Galaxies as Measured by WISE
• ALMA Observations of Multiple-CO and C Lines Toward the Active Galactic Nucleus of NGC 7469: X-Ray-dominated Region Caught in the Act
• Does the mid-infrared-hard X-ray luminosity relation for active galactic nuclei depend on Eddington ratio?
• Ultraluminous Infrared Galaxies in the AKARI All Sky Survey
• Search for Optically Dark Infrared Galaxies without Counterparts of Subaru Hyper Suprime-Cam in the AKARI North Ecliptic Pole Wide Survey Field
• The effect of the quasar H1821+643 on the surrounding intracluster medium: revealing the underlying cooling flow
• Evidence for a black hole in a radio-quiet quasar nucleus
• X-ray Emission from the Host Clusters of Powerful AGN
• The Relationship Between Brightest Cluster Galaxy Star Formation and the Intracluster Medium in CLASH
• Extreme conditions in the molecular gas of lensed star-forming galaxies at z~3
• Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\mathbf{z}\sim 4$: hidden AGN and star formation activity
• A Chandra HETG Observation of the Quasar H 1821+643 and Its Surrounding Cluster
• Dust Destruction by Charging: A Possible Origin of Grey Extinction Curves of Active Galactic Nuclei
• The X-ray spectrum of the cooling-flow quasar H1821+643 : A massive black hole feeding off the intracluster medium
• How unusual is the cool-core radio halo cluster CL1821+643 ?
• Dust Destruction by Drift-Induced Sputtering in Active Galactic Nuclei
• Unveiling the mask on the ULIRG-to-QSO transition object [H89]1821+643 at z=0.3: a gas-poor/gas-rich galaxy merger and the implications for CO-based dynamical mass estimates
• Analysis of Spitzer-IRS spectra of hyperluminous infrared galaxies
• An XMM-Newton study of Hyper-Luminous Infrared Galaxies
• Observational Evidence for Enhanced Black Hole Accretion in Giant Elliptical Galaxies
• Quenching of supermassive black hole growth around the apparent maximum mass
• Photometric observations of selected, optically bright quasars for Space Interferometry Mission and other future celestial reference frames

Cited by in corpus (1)

• Detection of the [O I] 63 $\mu$m emission line from the $z=6.04$ quasar J2054-0005