The First Chandra Field
arXiv:astro-ph/0509053 · doi:10.1086/497907
Abstract
Before the official first-light images, the Chandra X-Ray Observatory obtained an X-ray image of the field to which its focal plane was first exposed. We describe this historic observation and report our study of the first Chandra field. Chandra's Advanced CCD Imaging Spectrometer (ACIS) detected 15 X-ray sources, the brightest being dubbed ``Leon X-1'' to honor the Chandra Telescope Scientist, Leon Van Speybroeck. Based upon our analysis of the X-ray data and spectroscopy at the European Southern Observatory (ESO; La Silla, Chile), we find that Leon X-1 is a Type-1 (unobscured) active galactic nucleus (AGN) at a redshift z=0.3207. Leon X-1 exhibits strong Fe II emission and a broad-line Balmer decrement that is unusually flat for an AGN. Within the context of the Eigenvector-1 correlation space, these properties suggest that Leon X-1 may be a massive (> 10**{9} solar mass) black hole, accreting at a rate approaching its Eddington limit.
39 pages, 9 figures, accepted for publication in ApJ
References in corpus (21)
- On the Absorption of X-rays in the Interstellar Medium
- The USNO-B Catalog
- The XMM-Newton view of PG quasars I. X-ray continuum and absorption
- Eigenvector 1: An Optimal Correlation Space for Active Galactic Nuclei
- Nucleosynthesis and Mixing in Cassiopeia A
- The unusual emission line spectrum of IZw1
- XMM-Newton EPIC observations of 21 low-redshift PG quasars
- Chandra Discovery of a 100 kpc X-ray Jet in PKS 0637--752
- Searching for the Physical Drivers of the Eigenvector 1 Correlation Space
- Average Quasar Spectra in the Context of Eigenvector 1
- The Compact Central Object in Cas A: A Neutron Star with Hot Polar Caps or a Black Hole?
- Chandra X-ray Observations of the Spiral Galaxy M81
- Chandra Multi-wavelength Project (ChaMP). II. First Results of X-ray Source Properties
- Eddington Accretion and QSO Emission Lines at z ~ 2
- An Overview of the Performance of the Chandra X-Ray Observatory
- Spectroscopic Properties of QSOs Selected from Ultraluminous Infrared Galaxy Samples
- Radio Loud AGN in the Context of the Eigenvector 1 Parameter Space
- Chandra Observations of the Pleiades Open Cluster: X-ray Emission from Late-B to Early-F Type Binaries
- Searching for the Physical Drivers of Eigenvector-1: From Quasars to Nano-Quasars
- Two-temperature accretion flows in magnetic cataclysmic variables: Structures of post-shock emission regions and X-ray spectroscopy
- A complete sample of Seyfert galaxies selected at 1/4 keV