An Optical Catalog of the Chandra Large Area Synoptic X-ray Survey Sources
arXiv:astro-ph/0409088 · doi:10.1086/423998
Abstract
We present photometric and spectroscopic observations of the X-ray sources detected in the wide-area, moderately deep Chandra Large Area Synoptic X-ray Survey of the Lockman Hole-Northwest field. We have B, V, R, I, and z' photometry for 521 (99%) of the 525 sources in the X-ray catalog and spectroscopic redshifts for 271 (52%), including 20 stars. We do not find evidence for redshift groupings of the X-ray sources, like those found in the Chandra Deep Field surveys, because of the larger solid angle covered by this survey. We separate the X-ray sources by optical spectral type and examine the colors, apparent and absolute magnitudes, and redshift distributions for the broad-line and non-broad-line active galactic nuclei. Combining our wide-area survey with other Chandra and XMM-Newton hard X-ray surveys, we find a definite lack of luminous, high accretion rate sources at z<1, consistent with previous observations that showed that supermassive black hole growth is dominated at low redshifts by sources with low accretion rates.
arXiv comment35 pages, 12 figures, accepted for publication in the Astronomical Journal
References in corpus (42)
- The USNO-B Catalog
- New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
- The Chandra Deep Field-North Survey. XIII. 2 Ms Point-Source Catalogs
- Subaru Prime Focus Camera -- Suprime-Cam --
- The Chandra Deep Field South: the 1 Million Second
- Resolving the extragalactic hard X-ray background
- XMM-Newton observation of the Lockman Hole; I. The X-ray Data
- The Chandra Deep Field North Survey. V. 1 Ms Source Catalogs
- Optical and Infrared Properties of the 2 Ms Chandra Deep Field-North X-ray Sources
- A Deep, Wide Field, Optical, and Near Infrared Catalog of a Large Area around the Hubble Deep Field North
- The Team Keck Treasury Redshift Survey of the GOODS-North Field
- Study of the X-Ray Background Spectrum and its Large-Scale Fluctuation with ASCA
- The Chandra Deep Survey of the Hubble Deep Field North Area. II. Results from the Caltech Faint Field Galaxy Redshift Survey Area
- Radio sources in the 2dF Galaxy Redshift Survey - II. Local radio luminosity functions for AGN and star-forming galaxies at 1.4 GHz
- The HELLAS2XMM survey: IV. Optical identifications and the evolution of the accretion luminosity in the Universe
- X-ray, Optical, and Infrared Imaging and Spectral Properties of the 1 Ms Chandra Deep Field North Sources
- The Nature of the Hard X-ray Background Sources: Optical, Near-infrared, Submillimeter, and Radio Properties
- XMM-Newton observation of the Lockman Hole II. Spectral analysis
- New Results from the X-ray and Optical Survey of the Chandra Deep Field South: The 300ks Exposure
- A large sample of spectroscopic redshifts in the ACS-GOODS region of the HDF-N
- X-Rays from NGC 3256: High-Energy Emission in Starburst Galaxies and Their Contribution to the Cosmic X-Ray Background
- The Changing AGN Population
- The ROSAT Deep Survey: VI. X-ray sources and Optical identifications of the Ultra Deep Survey
- Tracing the large scale structure in the Chandra Deep Field South
- The HELLAS2XMM survey: I. The X-ray data and the Log(N)-Log(S)
- The Chandra Deep Field North Survey. XII. The Link Between Faint X-ray and Radio Source Populations
- Supermassive Black Hole Accretion History Inferred from a Large Sample of Chandra Hard X-ray Sources
- 2-8 keV X-ray number counts determined from Chandra blank field observations
- ROSAT and ASCA Observations of X-ray Luminous starburst Galaxies : NGC3310 and NGC3690
- The Chandra Deep Field-North Survey. XV. Optically Bright, X-ray Faint Sources
- Chandra Multi-wavelength Project (ChaMP). II. First Results of X-ray Source Properties
- Optical Identification of the ASCA Medium Sensitivity Survey in the Northern Sky: Nature of Hard X-ray-selected Luminous Active Galactic Nuclei
- The Evolution of the Ultraluminous Infrared Galaxy Population from Redshift 0 to 1.5
- The Chandra Deep Field North Survey. XI. X-ray emission from luminous infrared starburst galaxies
- Imaging Large Scale Structure in the X-ray Sky
- The Far-Infrared Spectral Energy Distributions of X-ray-selected Active Galaxies
- The Serendipitous Extragalactic X-Ray Source Identification (SEXSI) Program: I. Characteristics of the Hard X-Ray Sample
- SPICES II. Optical and Near-Infrared Identifications of Faint X-Ray Sources from Deep Chandra Observations of Lynx
- The Chandra Large Area Synoptic X-ray Survey (CLASXS) of the Lockman Hole-Northwest: The X-ray Catalog
- The deepest X-ray look at the Universe
- 172 ks Chandra Exposure of the LALA Boötes Field: X-ray Source Catalog
- The Composition of the Interstellar Medium towards the Lockman Hole. HI, UV and X-ray observations
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- Toward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations
- Luminosity-dependent evolution of soft X-ray selected AGN: New Chandra and XMM-Newton surveys
- The X-ray-to-Optical Properties of Optically-Selected Active Galaxies Over Wide Luminosity and Redshift Ranges
- The Cosmic Evolution of Hard X-ray Selected Active Galactic Nuclei
- X-ray spectral properties of AGN in the Chandra Deep Field South
- Absorption Properties and Evolution of Active Galactic Nuclei
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- The Luminosity Function of X-ray Selected Active Galactic Nuclei: Evolution of Supermassive Black Holes at High Redshift
- The Chandra COSMOS Survey: III. Optical and Infrared Identification of X-ray Point Sources
- Photometric redshifts in the SWIRE Survey
- The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources
- The Evolution of Obscuration in AGN
- Chandra Observations of the Highest Redshift Quasars from the Sloan Digital Sky Survey
- HELP: The Herschel Extragalactic Legacy Project
- The Unified Model of Active Galactic Nuclei: II. Evolutionary Connection
- The Population of High Redshift AGNs in the Chandra COSMOS survey
- The deepest X-ray view of high-redshift galaxies: constraints on low-rate black-hole accretion
- The Chandra XBootes Survey - III: Optical and Near-IR Counterparts
- The Resolved NIR Extragalactic Background
- The Resolved Near-Infrared Extragalactic Background
- Finding Rare AGN: XMM-Newton and Chandra Observations of SDSS Stripe 82
- The Serendipitous Extragalactic X-Ray Source Identification (SEXSI) Program. III. Optical Spectroscopy
- The OPTX Project II: Hard X-ray Luminosity Functions of Active Galactic Nuclei for z<5
- The OPTX Project I: The Flux and Redshift Catalogs for the CLANS, CLASXS, and CDF-N fields
- The Chandra Large Area Synoptic X-ray Survey (CLASXS) of the Lockman Hole-Northwest: The X-ray Catalog
- Spatial Correlation Function of the Chandra Selected Active Galactic Nuclei
- Evidence for an intermediate line region in AGN's inner torus region and its evolution from narrow to broad line Seyfert I galaxies
- Outshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904
- The HELLAS2XMM survey.VIII. Optical identifications of the extended sample
- Obscured and unobscured AGN populations in a hard-X-ray selected sample of the XMDS survey
- The X-ray luminosity function of AGN at z~3
- An Extremely Deep Wide-Field Near-Infrared Survey: Bright Galaxy Counts and Local Large Scale Structure
- The Number Density of Intermediate and High Luminosity Active Galactic Nuclei at z~2-3
- Chandra Multiwavelength Project: Normal Galaxies at Intermediate Redshift
- The OPTX Project III: X-ray versus Optical Spectral Type for AGNs
- Testing for a large local void by investigating the Near-Infrared Galaxy Luminosity Function
- BH Accretion in Low-Mass Galaxies Since z~1
- AGN dust tori: the X-ray-infrared connection
- The Stellar Population And Origin Of The Mysterious High-Latitude Star Forming Cloud CG 12
- Evolutionary Consequences of Dusty Tori in Active Galactic Nuclei
- Early Science Result from the Japanese Virtual Observatory: AGN and Galaxy Clustering at z = 0.3 to 3.0
- Evolution of supermassive black holes