A Quasar Catalog with Simultaneous UV, Optical and X-ray Observations by Swift
arXiv:1203.6071 · doi:10.1088/0067-0049/201/2/10
Abstract
We have compiled a catalog of optically-selected quasars with simultaneous observations in UV/optical and X-ray bands by the Swift Gamma Ray Burst Explorer. Objects in this catalog are identified by matching the Swift pointings with the Sloan Digital Sky Survey Data Release 5 quasar catalog. The final catalog contains 843 objects, among which 637 have both UVOT and XRT observations and 354 of which are detected by both instruments. The overall X-ray detection rate is ~60% which rises to ~85% among sources with at least 10 ks of XRT exposure time. We construct the time-averaged spectral energy distribution for each of the 354 quasars using UVOT photometric measurements and XRT spectra. From model fits to these SEDs, we find that the big blue bump contributes about 0.3 dex to the quasar luminosity. We re-visit the alpha_ox-L_uv relation by selecting a clean sample with only type 1 radio-quiet quasars; the dispersion of this relation is reduced by at least 15% compared to studies that use non-simultaneous UV/optical and X-ray data. We only found a weak correlation between L/L_Edd and alpha_uv. We do not find significant correlations between alpha_x and alpha_ox, alpha_ox and alpha_uv, and alpha_x and Log L(0.3-10 keV). The correlations between alpha_uv and alpha_x, alpha_ox and alpha_x, alpha_ox and alpha_uv, L/L_Edd and alpha_x, and L/L_Edd and alpha_ox are stronger amongst low-redshift quasars, indicating that these correlations are likely driven by the changes of SED shape with accretion state.
63 pages, 22 figures, accepted by ApJS
References in corpus (34)
- The X-ray-to-Optical Properties of Optically-Selected Active Galaxies Over Wide Luminosity and Redshift Ranges
- Biases in Virial Black Hole Masses: An SDSS Perspective
- The Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release
- CRATES: An All-Sky Survey of Flat-Spectrum Radio Sources
- The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky Survey
- Roma-BZCAT: A multifrequency catalogue of Blazars
- A Catalog of Broad Absorption Line Quasars in Sloan Digital Sky Survey Data Release 5
- Simultaneous X-ray/optical/UV snapshots of active galactic nuclei from XMM-Newton: spectral energy distributions for the reverberation mapped sample
- A Comprehensive Study of 2 000 Narrow Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey: I. The Sample
- Radio-loud Narrow-Line Type 1 Quasars
- Swift BAT Survey of AGN
- The Hard X-ray Spectrum as a Probe for Black-Hole Growth in Radio-Quiet Active Galactic Nuclei
- The Hard X-ray Spectral Slope as an Accretion-Rate Indicator in Radio-Quiet Active Galactic Nuclei
- Suzaku Observations of Active Galactic Nuclei Detected in the Swift/BAT Survey: Discovery of "New Type" of Buried Supermassive Black Holes
- The First Swift Ultra-Violet/Optical Telescope GRB Afterglow Catalog
- FIRST `Winged' and `X'-shaped Radio Source Candidates
- Long-Term Profile Variability of Double Peaked Emission Lines in Active Galactic Nuclei
- Quasi-Periodic Oscillations of ~ 15 minutes in the Optical Light Curve of the BL Lac S5 0716+714
- The Black Hole-Bulge Relationship in Luminous Broad-Line Active Galactic Nuclei and Host Galaxies
- XMM-Newton observations of the Narrow-Line Seyfert 1 galaxy Mrk 335 in an historical low X-ray flux state
- Spectral variability of quasars from multi-epoch photometric data in the Sloan Digital Sky Survey Stripe 82
- Variable VHE gamma-ray emission from non-blazar AGNs
- A Large Sample of BL Lacs from SDSS and FIRST
- The Variable X-ray Spectrum of Markarian 766 - II. Time-Resolved Spectroscopy
- The X-ray Properties of Early-Type Galaxies in the Extended Chandra Deep Field-South
- Evolution of the X-ray Emission of Radio-Quiet Quasars
- Variability of Active Galactic Nuclei from the Optical to X-ray Regions
- The Sloan Digital Sky Survey Quasar Lens Search. IV. Statistical Lens Sample from the Fifth Data Release
- AEGIS: A Multi-wavelength Study of Spitzer Power-law Galaxies
- Discovery of an Extreme MeV Blazar with the Swift Burst Alert Telescope
- A Chandra Survey of the X-ray Properties of Broad Absorption Line Radio-Loud Quasars
- The X-ray Properties of Active Galactic Nuclei with Double-Peaked Balmer Lines
- Chandra Observations of Red Sloan Digital Sky Survey Quasars
- Lensed Image Angles: New Statistical Evidence for Substructure
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- Correlation between the photon index and X-ray luminosity of black hole X-ray binaries and active galactic nuclei: observations and interpretation
- The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-Look Quasars
- An X-ray/SDSS sample (I): multi-phase outflow incidence and dependence on AGN luminosity
- X-ray Properties of Intermediate-mass Black Holes in Active Galaxies. III. Spectral Energy Distribution and Possible Evidence for Intrinsically X-ray-weak AGNs
- On the Observational Difference Between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei
- The X-ray and Mid-Infrared luminosities in Luminous Type 1 Quasars
- Variability and the X-ray/UV ratio of active galactic nuclei. II. Analysis of a low-redshift Swift sample
- A Uniformly Selected Sample of Low-Mass Black Holes in Seyfert 1 Galaxies. II. The SDSS DR7 Sample
- X-rays from the redshift 7.1 quasar ULAS J1120+0641
- A New Method to Measure Star Formation Rates in Active Galaxies Using Mid-infrared Neon Emission Lines
- An optical overview of blazars with LAMOST I: Hunting changing-look blazars and new redshift estimates
- An X-ray/SDSS sample (II): outflowing gas plasma properties
- A catalog of optical to X-ray spectral energy distributions of z~2 quasars observed with Swift. I: First results
- The Starburst-AGN connection: quenching the fire and feeding the beast
- Unveiling the Universe with Emerging Cosmological Probes
- Radio recombination lines from obscured quasars with the SKA
- Swift Monitoring Observations of Mrk 231: Detection of Ultraviolet Variability
- Gemini Near Infrared SpectrographDistant Quasar Survey: the Chandra View
- Can X-ray Observations Improve Optical-UV-based Accretion-Rate Estimates for Quasars?