GALEX far-UV color selection of UV-bright high-redshift quasars
arXiv:1004.3347 · doi:10.1088/0004-637X/728/1/23
Abstract
We study the small population of z>2.7 quasars detected by GALEX, whose far-UV emission is not extinguished by intervening HI Lyman limit systems. These quasars are of particular importance to detect intergalactic HeII absorption along their sightlines. We correlate verified z>2.7 quasars to the GALEX GR4 source catalog, yielding 304 S/N>3 sources. However, ~50% of these are only detected in the GALEX NUV band, signaling the truncation of the FUV flux by low-redshift Lyman limit systems. We exploit the GALEX UV color to cull the most promising targets for follow-up studies, with blue (red) GALEX colors indicating transparent (opaque) sightlines. Monte Carlo simulations indicate a HeII detection rate of ~60% for quasars with FUV-NUV<1 at z<3.5, a ~50% increase over GALEX searches that do not include color information. We regard 52 quasars detected at S/N>3 to be most promising for HST follow-up, with an additional 114 quasars if we consider S/N>2 detections in the FUV. SDSS provides just half of the NUV-bright quasars that should have been detected by SDSS & GALEX. We revise the SDSS quasar selection function, finding that SDSS systematically misses quasars with blue u-g<2 colors at 3<z<3.5 due to overlap with the stellar locus in color space. Our color-dependent SDSS selection function naturally explains the inhomogeneous u-g color distribution of SDSS quasars with redshift and the color difference between color-selected and radio-selected SDSS quasars. Moreover, it yields excellent agreement between the observed and the predicted number of UV-bright SDSS quasars. We confirm our previous claims that SDSS preferentially selects 3<z<3.5 quasars with intervening HI Lyman limit systems. Our results imply that broadband optical color surveys for 3<z<3.5 quasars have likely underestimated their space density by selecting IGM sightlines with an excess of strong HI absorbers.
22 pages, 17 figures, accepted for publication in ApJ. Figure 1 replaced and Section 2 expanded, Tables 3 and 4 included, conclusions unchanged
References in corpus (26)
- The Sloan Digital Sky Survey Quasar Catalog V. Seventh Data Release
- A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
- The Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release
- HeII Reionization and its Effect on the IGM
- A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2
- The Evolution of Lyman Limit Absorption Systems to Redshift Six
- A Definitive Survey for Lyman Limit Systems at z~3.5 with the Sloan Digital Sky Survey
- An improved measurement of the flux distribution of the Ly-alpha forest in QSO absorption spectra: the effect of continuum fitting, metal contamination and noise properties
- Physical Properties, Baryon Content, and Evolution of the LyαForest: New Insights from High Resolution Observations at z < 0.4
- Voigt Profile Fitting to Quasar Absorption Lines: An Analytic Approximation to the Voigt-Hjerting Function
- The Keck+Magellan Survey for Lyman Limit Absorption I: The Frequency Distribution of Super Lyman Limit Systems
- An unbiased measurement of the UV background and its evolution via the proximity effect in quasar spectra
- A Monte Carlo simulation of the intergalactic absorption and the detectability of the Lyman continuum from distant galaxies
- Statistical Properties of the GALEX/SDSS matched source catalogs, and classification of the UV sources
- The UV spectrum of HS1700+6416 II. FUSE observations of the HeII Lyman alpha forest
- Reionisation scenarios and the temperature of the IGM
- Photo-heating and the fate of hard photons during the reionisation of HeII by quasars
- The Evolution of Lyman alpha Absorbers in the Redshift Range 0.5<z<1.9
- GALEX-SDSS Catalogs for Statistical Studies
- Continuous statistics of the Lyman-alpha forest at 0 < z < 1.6: the mean flux, flux distribution, and autocorrelation from HST FOS spectra
- The Faint End of the Quasar Luminosity Function at z~4
- Spectral shape of the UV ionizing background and HeII absorption at redshifts 1.8 < z < 2.9
- Fluctuations in the Ionizing Background During and After Helium Reionization
- A High Yield of New Sightlines for the Study of Intergalactic Helium: Far-UV-Bright Quasars from SDSS, GALEX, and HST
- Fluctuations of the intergalactic UV background towards two lines of sight
- Deep GALEX Observations of the Coma Cluster: Source Catalog and Galaxy Counts
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- Active Galactic Nuclei: what's in a name?
- The Evolution of the Intergalactic Medium
- The SDSS-III Baryon Oscillation Spectroscopic Survey: Quasar Target Selection for Data Release Nine
- Discovery of three z>6.5 quasars in the VISTA Kilo-degree Infrared Galaxy (VIKING) survey
- The Sloan Digital Sky Survey quasar catalog: ninth data release
- The first ultraviolet quasar stacked spectrum at z=2.4 from WFC3
- Evolution of the AGN UV luminosity function from redshift 7.5
- The z=5 Quasar Luminosity Function from SDSS Stripe 82
- Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6
- Think Outside the Color Box: Probabilistic Target Selection and the SDSS-XDQSO Quasar Targeting Catalog
- The SDSS-III Baryon Oscillation Spectroscopic Survey: The Quasar Luminosity Function from Data Release Nine
- The Giant Gemini GMOS survey of z>4.4 quasars - I. Measuring the mean free path across cosmic time
- A Refined Measurement of the Mean Transmitted Flux in the Ly-alpha Forest over 2 < z < 5 Using Composite Quasar Spectra
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- A Principal Component Analysis of quasar UV spectra at z~3
- AGNfitter: A Bayesian MCMC approach to fitting spectral energy distributions of AGN
- Early and Extended Helium Reionization Over More Than 600 Million Years of Cosmic Time
- The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars
- XQ-100: A legacy survey of one hundred 3.5 < z < 4.5 quasars observed with VLT/XSHOOTER
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- The End of Helium Reionization at z~2.7 Inferred from Cosmic Variance in HST/COS HeII Lyman Alpha Absorption Spectra
- The Faint End of the z=5 Quasar Luminosity Function from the CFHTLS
- Variability selected high-redshift quasars on SDSS Stripe 82
- The HST/ACS+WFC3 Survey for Lyman Limit Systems II: Science
- IGM Constraints from the SDSS-III/BOSS DR9 Ly-alpha Forest Flux Probability Distribution Function
- A survey of luminous high-redshift quasars with SDSS and WISE II. the bright end of the quasar luminosity function at z ~ 5
- The imprint of inhomogeneous HeII reionization on the HI and HeII Ly-alpha forest
- Confronting Simulations of Optically Thick Gas in Massive Halos with Observations at z=2-3
- The evolution of neutral gas in damped Lyman systems from the XQ-100 survey
- Precious Metals in SDSS Quasar Spectra I: Tracking the Evolution of Strong, 1.5 < z < 4.5 CIV Absorbers with Thousands of Systems
- The Magellan Uniform Survey of Damped Lyman alpha Systems I: Cosmic Metallicity Evolution
- Bayesian High-Redshift Quasar Classification from Optical and Mid-IR Photometry
- A New Precision Measurement of the Small-Scale Line-of-Sight Power Spectrum of the Ly Forest
- VLT LBG Redshift Survey II: Interactions between galaxies and the IGM at z ~3
- The Clustering of High-Redshift (2.9 z 5.1) Quasars in SDSS Stripe 82
- Statistical properties of damped Lyman-alpha systems from Sloan Digital Sky Survey DR12
- Mean and Extreme Radio Properties of Quasars and the Origin of Radio Emission
- Statistical Detection of the HeII Transverse Proximity Effect: Evidence for Sustained Quasar Activity for 25 Million Years
- Efficient Selection of Quasar Candidates Based on Optical and Infrared Photometric Data Using Machine Learning
- Two more, bright, z > 6 quasars from VST ATLAS and WISE
- The Evolution of the HeII-Ionizing Background at Redshifts 2.3<z<3.8 Inferred from a Statistical Sample of 24 HST/COS HeII Ly Absorption Spectra
- Discovery of a Radio-Selected z ~ 6 Quasar
- The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey footprint. III. The South Galactic Cap Sample and the Quasar Luminosity Function at Cosmic Noon
- Strong Clustering of Lyman Break Galaxies around Luminous Quasars at z~4
- AGN-driven helium reionization and the incidence of extended HeIII regions at redshift z>3
- HST/COS Observations of Thirteen New He II Quasars
- The Extremely Luminous Quasar Survey in the Pan-STARRS 1 Footprint (PS-ELQS)
- Clustering of Lyman-alpha Emitters Around Quasars at
- A self-consistent 3D model of fluctuations in the helium-ionizing background
- The Effect of Fluctuations on the Helium-Ionizing Background
- Cosmological Constraints from the eBOSS Lyman- Forest using the PRIYA Simulations
- New Evidence for Extended HeII Reionization at z>3.5 from HeII Lyman Alpha and Beta Transmission Spikes
- The spectral and environment properties of quasar pairs
- Dating individual quasars with the HeII proximity effect
- The Astrophysical Consequences of Intervening Galaxy Gas on Fast Radio Bursts
- Detecting Multiple DLAs per Spectrum in SDSS DR12 with Gaussian Processes
- The Extremely Luminous Quasar Survey (ELQS) in the Sloan Digital Sky Survey footprint. II. The North Galactic Cap Sample
- Streamlined Lensed Quasar Identification in Multiband Images via Ensemble Networks
- Imprints of the first billion years: Lyman limit systems at
- Paving the Way for Euclid and JWST via Optimal Selection of High-z Quasars
- Detecting neutral hydrogen at z > 3 in large spectroscopic surveys of quasars
- When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multi-band Imaging Data
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