The gravitationally lensed, luminous infrared galaxy IRAS F10214+4724 observed with XMM-Newton
arXiv:0905.3512 · doi:10.1016/j.newast.2009.05.009
Abstract
We report on a short XMM-Newton observation of the gravitationally-lensed, luminous infrared galaxy IRAS F10214+4724 at z=2.3. A faint X-ray source is detected at 4 sigma. The observed 0.5-2 keV (1.7-6.6 keV in the rest-frame) flux is 1.3e-15 erg/s/cm2 and the spectral slope in the rest-frame 1-10 keV band is Gamma~2. These results agree with those obtained from the Chandra X-ray Observatory, given the large uncertainties in both measurements. While possible evidence for excess emission above 5 keV is seen, we suspect this excess might be either spurious or not related to the infrared galaxy.
arXiv comment4 pages, 2 figures, New Astronomy in press
References in corpus (16)
- The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
- Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background
- Observations of Ultraluminous Infrared Galaxies with the Infrared Spectrograph on the Spitzer Space Telescope II: The IRAS Bright Galaxy Sample
- Spitzer Quasar and ULIRG evolution study (QUEST): I. The origin of the far infrared continuum of QSOs
- Aromatic Features in AGN: Star-Forming Infrared Luminosity Function of AGN Host Galaxies
- A Gravitational Lens Solution for IRAS F10214+4724
- HST Observations of the Luminous IRAS Source FSC10214+4724: A Gravitationally Lensed Infrared Quasar
- New Observations and a New Interpretation of CO(3--2) in IRAS F10214+4724
- Silicate Emission in the Spitzer IRS spectrum of FSC 10214+4724
- Atomic Carbon in APM 08279+5255 at z=3.91
- A model for the infrared emission of FSC 10214+4724
- The CO line SED and atomic carbon in IRAS F10214+4724
- A Chandra observation of the z=2.285 galaxy FSC10214+4724: Evidence for a Compton-thick quasar?
- IRAS F10214+4724: the inner 100pc
- An X-ray bright ERO hosting a type 2 QSO
- How much of the extreme luminosity of IRAS F10214+4724 can be attributed to gravitational lensing