Host Galaxies of Hard X-ray Selected Type-2 Active Galactic Nuclei at Intermediate Redshifts
arXiv:astro-ph/0604291 · doi:10.1086/505108
Abstract
We study properties of the host galaxies of 15 hard X-ray selected type-2 active galactic nuclei (AGNs) at intermediate redshifts (0.050.6) detected in surveys. The absorption corrected hard X-ray luminosities range from 10 erg s to erg s. We took the -band image of these AGNs with the University of Hawaii 2.2 m telescope. Thanks to the intrinsic obscuration of nuclear light, we can decompose the galaxies with a spheroid component and a disk component. The resulting spheroid luminosities correlate with ; higher (lower) X-ray luminosity AGNs tend to reside in luminous (less luminous) spheroids. It is also found that the hosts of luminous AGNs show a large spheroid-to-disk luminosity ratio (1), while those of less luminous AGNs spread between 0 and 1. The correlation between and spheroid luminosity indicates that the relation between mass of a supermassive black hole (SMBH) and spheroid luminosity (BS-relation) at the intermediate redshifts. The BS-relation agrees with that in the local universe if the Eddington ratio of 0.24 is adopted, which is a mean value determined from our type-1 AGN sample at similar redshifts through the broad-line width and continuum luminosity. The present study demonstrates the effectiveness of using type-2 AGNs at high redshifts to study their host properties.
arXiv comment21 pages, 8 figures, ApJ accepted
References in corpus (25)
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- The Demography of Massive Dark Objects in Galaxy Centres
- Detailed Structural Decomposition of Galaxy Images
- Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei
- The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
- Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background
- Cosmological Evolution of the Hard X-ray AGN Luminosity Function and the Origin of the Hard X-ray Background
- Luminosity-dependent evolution of soft X-ray selected AGN: New Chandra and XMM-Newton surveys
- On the black hole - bulge mass relation in active and inactive galaxies
- Quasars, their host galaxies, and their central black holes
- Black Hole Mass Estimates from Reverberation Mapping and from Spatially Resolved Kinematics
- The HELLAS2XMM survey. VII. The hard X-ray luminosity function of AGN up to z=4: more absorbed AGN at low luminosities and high redshifts
- Super-massive Black Hole Demography: the Match between the Local and Accreted Mass Functions
- Black Hole Demographics from the M(BH)-sigma Relation
- The Black Hole-Bulge Relationship in QSOs
- The Relationship Between Stellar and Black-Hole Mass in Submillimeter Galaxies
- Colors of AGN host galaxies at 0.5<z<1.1 from GEMS
- Probing the Coevolution of Supermassive Black Holes and Quasar Host Galaxies
- Optical Identification of the ASCA Large Sky Survey
- Quasar host galaxy star formation activity from multicolour data
- The ASCA Medium Sensitivity Survey (the GIS Catalog Project): Source Counts and Evidence for Emerging Population of Hard Sources
- Optical Identification of the ASCA Medium Sensitivity Survey in the Northern Sky: Nature of Hard X-ray-selected Luminous Active Galactic Nuclei
- Supermassive Black Hole Mass Functions at Intermediate Redshifts from Spheroid and AGN Luminosity Functions
- Host Galaxies of the High-redshift AGNs in the GOODS Fields
- Near-Infrared Colors of Hard X-ray Selected Active Galactic Nuclei
Cited by in corpus (4)
- A New Sample of Buried Active Galactic Nuclei Selected from the Second XMM-Newton Serendipitous Source Catalogue
- Accretion Properties of A Sample of Hard X-ray (<60keV) Selected Seyfert 1 Galaxies
- Physical Properties, Star Formation, and Active Galactic Nucleus Activity in Balmer Break Galaxies at 0 < z < 1
- First Detection of 12CO (1--0) Emission from Two Narrow-Line Seyfert 1 Galaxies