A Chandra observation of the z=2.285 galaxy FSC10214+4724: Evidence for a Compton-thick quasar?
arXiv:astro-ph/0411289 · doi:10.1111/j.1745-3933.2005.08621.x
Abstract
We present a ~20 ks Chandra ACIS-S observation of the strongly lensed z=2.285 ultra-luminous infrared galaxy FSC10214+4724. Although this observation achieves the equivalent sensitivity of an up-to ~4 Ms Chandra exposure (when corrected for gravitational lensing), the rest-frame 1.6-26.3 keV emission from FSC10214+4724 is weak (L_X~2E42 erg/s for a lensing boost of ~100); a significant fraction of this X-ray emission appears to be due to vigorous star-formation activity. If FSC10214+4724 hosts a quasar, as previously suggested, then it must be obscured by Compton-thick material. We compare FSC10214+4724 to high-redshift SCUBA galaxies and discuss the X-ray identification of Compton-thick AGNs at high redshift.
arXiv comment5 pages, 3 figures; MNRAS letters, in press
References in corpus (33)
- The Second Data Release of the Sloan Digital Sky Survey
- Astrometric Calibration of the Sloan Digital Sky Survey
- Submillimeter Galaxies
- The Chandra Deep Field-North Survey. XIII. 2 Ms Point-Source Catalogs
- The 2-10 keV luminosity as a Star Formation Rate indicator
- A Wavelet-Based Algorithm for the Spatial Analysis of Poisson Data
- A 3 dimensional diagnostic diagram for Seyfert 2s: probing X-ray absorption and Compton thickness
- The nature of faint submm-selected galaxies
- A median redshift of 2.4 for galaxies bright at submillimetre wavelengths
- Deep radio imaging of the SCUBA 8-mJy survey fields: sub-mm source identifications and redshift distribution
- Clustering of Submillimeter-Selected Galaxies
- The Fall of AGN and the Rise of Star-Forming Galaxies: A Close Look at the Chandra Deep Field X-ray Number Counts
- Near-infrared template spectra of normal galaxies: k-corrections, galaxy models and stellar populations
- X-ray Observations of Optically-Selected, Radio-Quiet Quasars I: The ASCA results
- Interferometric Observations of Powerful CO Emission from the three Submillimeter Galaxies at z=2.30, 2.51 and 3.35
- Hyperluminous Infrared Galaxies
- The Chandra Deep Field-North Survey. XIV. X-ray detected Obscured AGNs and Starburst Galaxies in the Bright Submm Source Population
- Evidence for extended, obscured starbursts in submm galaxies
- Mitigating Charge Transfer Inefficiency in the Chandra X-ray Observatory's ACIS Instrument
- The Chandra Deep Field North Survey. XII. The Link Between Faint X-ray and Radio Source Populations
- A Gravitational Lens Solution for IRAS F10214+4724
- HST Observations of the Luminous IRAS Source FSC10214+4724: A Gravitationally Lensed Infrared Quasar
- A multivariate statistical analysis of spiral galaxy luminosities. I. Data and results
- New Observations and a New Interpretation of CO(3--2) in IRAS F10214+4724
- Chandra detection of reflected X-ray emission from the type 2 QSO in IRAS 09104+4109
- The intrinsic emission of Seyfert galaxies observed with BeppoSAX/PDS I. Comparison of the average spectra of the three classes of Seyfert Galaxies
- On the detectability of distant Compton-thick obscured quasars
- Dust Enshrouded AGN Models for Hyperluminous High Redshift IR Galaxies
- XMM-Newton observations of two hyperluminous IRAS galaxies: Compton-thick quasars with obscuring starbursts
- A spectroscopic study of IRAS F10214+4724
- IRAS F10214+4724: the inner 100pc
- How much of the extreme luminosity of IRAS F10214+4724 can be attributed to gravitational lensing
- HST Imaging Polarimetry of the Gravitational Lens FSC10214+4724
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- The evolution of AGN across cosmic time: what is downsizing?
- The obscuration by dust of most of the growth of supermassive black holes
- Reliable Identification of Compton-thick Quasars at z~2: Spitzer Mid-IR spectroscopy of HDF-oMD49
- A population of high-redshift type-2 quasars-I. Selection Criteria and Optical Spectra
- Molecules in galaxies
- A submm survey of Lyman-alpha haloes in the SA22 protocluster at z=3.1
- NuSTAR Observations of Heavily Obscured Quasars at z ~ 0.5
- A CANDELS WFC3 Grism Study of Emission-Line Galaxies at z~2: A Mix of Nuclear Activity and Low-Metallicity Star Formation
- X-ray Spectral Constraints for z~2 Massive Galaxies: The Identification of Reflection-Dominated Active Galactic Nuclei
- Evidence for a large fraction of Compton-thick quasars at high redshift
- Silicate Emission in the Spitzer IRS spectrum of FSC 10214+4724
- Obscured and unobscured AGN populations in a hard-X-ray selected sample of the XMDS survey
- Active galactic nucleus torus models and the puzzling infrared spectrum of IRAS F10214+4724
- Obscured and powerful AGN and starburst activities at z~3.5
- X-rays from the Type II quasar in the hyperluminous infrared galaxy IRAS F15307+3252
- Discovery of Compton-thick quasars in the Sloan Digital Sky Survey
- The preferentially magnified active nucleus in IRAS F10214+4724 - III. VLBI observations of the radio core
- Chandra X-ray observations of the hyper-luminous infrared galaxy IRAS F15307+3252
- The preferentially magnified active nucleus in IRAS F10214+4724 - I. Lens model and spatially resolved radio emission
- Most supermassive black hole growth is obscured by dust
- The gravitationally lensed, luminous infrared galaxy IRAS F10214+4724 observed with XMM-Newton
- SOFIA/HAWC+ detection of a gravitationally lensed starburst galaxy at = 1.03