An unbiased measurement of the UV background and its evolution via the proximity effect in quasar spectra
arXiv:0807.5089 · doi:10.1051/0004-6361:200810724
Abstract
We used 40 high resolution, high S/N QSO spectra at 2.1<z<4.7 to search for the signature of the proximity effect in the HI Lyalpha forest. Comparing the effective optical depth near each QSO with the expected one, we clearly detect the proximity effect on the combined QSO sample and towards each individual QSO. The observed proximity effect strength distribution (PESD) is asymmetric towards a weak effect. We demonstrate that this is not simply an effect of gravitational clustering around QSOs. Comparing simulated PESDs with observations, we argue that the averaging method to determine the UVB intensity J is heavily biased towards high values because of the PESD asymmetry. Using instead the mode of the PESD provides an unbiased estimate of J. For our sample its modal value is log(J)=-21.51+/-0.15 (in units of ergcm^-2s^-1Hz^-1sr^-1) at z=2.73. We estimated the excess HI absorption attributed to gravitational clustering. On scales of ~3 Mpc, only a minority of QSOs shows overdensities of up to a factor of a few in tau_eff; these are exactly the objects with the weakest proximity effects. After removing them, we redetermined the UVB intensity arriving at log(J)=-21.46+0.14-0.21. This is the most accurate measurement of J to date. We present a new diagnostic based on the shape of the PESD which strongly supports our conclusion that there is no systematic overdensity bias for the proximity effect. This additional diagnostic breaks the otherwise unavoidable degeneracy of the proximity effect between UVB and overdensity. We estimated the redshift evolution of J and found tentative evidence for a mild decrease with increasing redshift. Our results are in excellent agreement with predictions for the evolving UVB intensity, supporting the notion of a substantial contribution of star-forming galaxies.
arXiv comment20 pages, 19 figures (2 in Appendix), abridged abstract. Accepted by A&A, following the referee report
References in corpus (45)
- Composite Quasar Spectra From the Sloan Digital Sky Survey
- Radiative Transfer in a Clumpy Universe: II. The Utraviolet Extragalactic Background
- An Observational Determination of the Bolometric Quasar Luminosity Function
- Radiative Transfer in a Clumpy Universe: III. The Nature of Cosmological Ionizing Sources
- The Rest-Frame Extreme Ultraviolet Spectral Properties of QSOs
- The Lyman Alpha Forest in the Spectra of QSOs
- The Low Redshift Lyman Alpha Forest in Cold Dark Matter Cosmologies
- Metallicity of the intergalactic medium using pixel statistics. II. The distribution of metals as traced by C IV
- The Opacity of the Lyman Alpha Forest and Implications for Omega_{baryon} and the Ionizing Background
- The Linear Theory Power Spectrum from the Lyman-alpha Forest in the Sloan Digital Sky Survey
- P3M-SPH simulations of the Lyman-alpha Forest
- Broad Emission Line Shifts in Quasars: An Orientation Measure for Radio-Quiet Quasars?
- The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyman-alpha Forest
- The Direct Detection of Lyman-Continuum Emission from Star-forming Galaxies at z~3
- A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2
- The Distribution of Column Densities and b Values in the Lyman-Alpha Forest
- The evolution of faint AGN between z~1 and z~5 from the COMBO-17 survey
- The Lyman-alpha forest opacity and the metagalactic hydrogen ionization rate at z~2-4
- A Uniform Analysis of the Ly-alpha forest at z = 0 - 5: II. Measuring the mean intensity of the extragalactic ionizing background using the proximity effect
- The High-Redshift He II Gunn-Peterson Effect: Implications and Future Prospects
- 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
- The physical properties of the Ly-Alpha forest at z > 1.5
- The power spectrum of the flux distribution in the Lyman-alpha forest of a Large sample of UVES QSO Absorption Spectra (LUQAS)
- The Lyman-Alpha Forest at 1.5 < z < 4
- The effects of UV background correlations on LyA forest flux statistics
- The H I opacity of the intergalactic medium at redshifts 1.6 < z < 3.2
- Cosmological parameters sigma_8, the baryon density, and the UV background intensity from a calibrated measurement of H I Lyman-alpha absorption at z = 1.9
- A feature at z ~ 3.2 in the evolution of the Ly-alpha forest optical depth
- The Proximity Effect, the UV Background and the Statistics of the Lyman-Alpha Lines at High Resolution
- The faint end of the QSO luminosity function at z=3
- A Flat Photoionization Rate at 2<z<4.2: Evidence for a Stellar-Dominated UV Background and Against a Decline of Cosmic Star Formation Beyond z~3
- The Optical - Infrared Colors of CORALS QSOs: Searching for Dust Reddening Associated With High Redshift Damped Lyman Alpha Systems
- Faint AGN and the Ionizing Background
- The Transverse Proximity Effect: A Probe to the Environment, Anisotropy, and Megayear Variability of QSOs
- Evolution of the Ionizing Background at High Redshifts
- A Uniform Analysis of the Ly-alpha Forest at z=0 - 5: V. The extragalactic ionizing background at low redshift
- The Space Distribution of the Lyman Alpha Clouds in the Line of Sight to the Z=3.66 QSO 0055-269
- A Concordance Model of the Lyman-alpha Forest at z = 1.95
- Probing Early Clustering with Lyman-Alpha Absorption Lines Beyond the Quasar Redshift
- The proximity effect in a close group of QSOs
- The density structure around quasars from optical depth statistics
- The Line-of-Sight Proximity Effect and the Mass of Quasar Host Halos
- Spectral energy distribution of the metagalactic ionizing radiation field from QSO absorption spectra
- Analysis of Ly absorption lines in the vicinity of QSOs
- The line-of-sight proximity effect in individual quasar spectra
Cited by in corpus (79)
- New Measurements of the Ionizing Ultraviolet Background over 2 < z < 5 and Implications for Hydrogen Reionization
- Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7
- Hydrogen reionisation ends by : Lyman- optical depth measured by the XQR-30 sample
- The Giant Gemini GMOS survey of z>4.4 quasars - I. Measuring the mean free path across cosmic time
- Correcting CIV-Based Virial Black Hole Masses
- The optically unbiased GRB host (TOUGH) survey. I. Survey design and catalogs
- A Refined Measurement of the Mean Transmitted Flux in the Ly-alpha Forest over 2 < z < 5 Using Composite Quasar Spectra
- Measurements of the UV background at 4.6 < z < 6.4 using the quasar proximity effect
- New Constraints on IGM Thermal Evolution from the Lyα Forest Power Spectrum
- A Definitive Survey for Lyman Limit Systems at z~3.5 with the Sloan Digital Sky Survey
- New synthesis models of consistent extragalactic background light over cosmic time
- GeV Gamma-Ray Attenuation and the High-Redshift UV Background
- A Measurement of Small Scale Structure in the 2.2 < z < 4.2 Lyman-alpha Forest
- An X-shooter composite of bright 1 < z < 2 quasars from UV to infrared
- Quasars Probing Quasars VI. Excess HI Absorption Within One Proper Mpc of z~2 Quasars
- A Direct Measurement of the IGM Opacity to HI Ionizing Photons
- Large Fluctuations in the High-Redshift Metagalactic Ionizing Background
- Detection of dark galaxies and circum-galactic filaments fluorescently illuminated by a quasar at z=2.4
- A Principal Component Analysis of quasar UV spectra at z~3
- Early and Extended Helium Reionization Over More Than 600 Million Years of Cosmic Time
- The photoheating of the intergalactic medium in synthesis models of the UV background
- XQ-100: A legacy survey of one hundred 3.5 < z < 4.5 quasars observed with VLT/XSHOOTER
- Dissecting the properties of optically-thick hydrogen at the peak of cosmic star formation history
- The End of Helium Reionization at z~2.7 Inferred from Cosmic Variance in HST/COS HeII Lyman Alpha Absorption Spectra
- 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
- The intergalactic medium thermal history at redshift z=1.7--3.2 from the Lyman alpha forest: a comparison of measurements using wavelets and the flux distribution
- MApping the Most Massive Overdensities Through Hydrogen (MAMMOTH) I: Methodology
- Predicting Quasar Continua Near Lyman- with Principal Component Analysis
- A New Measurement of the Temperature Density Relation of the IGM From Voigt Profile Fitting
- The imprint of inhomogeneous HeII reionization on the HI and HeII Ly-alpha forest
- GALEX far-UV color selection of UV-bright high-redshift quasars
- A New Precision Measurement of the Small-Scale Line-of-Sight Power Spectrum of the Ly Forest
- Measurement of the small-scale structure of the intergalactic medium using close quasar pairs
- The evolution of HI and CIV quasar absorption line systems at 1.9 < z < 3.2
- A comparison of quasar emission reconstruction techniques for Lyman- and Lyman- transmission
- A High Signal-to-Noise Ratio Composite Spectrum of Gamma-ray Burst Afterglows
- The first measurement of the quasar lifetime distribution
- Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
- The Lyman alpha forest flux probability distribution at z>3
- Statistical Detection of the HeII Transverse Proximity Effect: Evidence for Sustained Quasar Activity for 25 Million Years
- Dark Galaxy Candidates at Redshift ~3.5 Detected with MUSE
- The Keck+Magellan Survey for Lyman Limit Absorption II: A Case Study on Metallicity Variations
- Helium Reionization Simulations. II. Signatures of Quasar Activity on the IGM
- The evolution of the helium-ionizing background at z ~ 2-3
- Constraining the lifetime and opening angle of quasars using fluorescent Lyman emission: the case of Q0420-388
- The Effect of Fluctuations on the Helium-Ionizing Background
- Modeling the HeII Transverse Proximity Effect: Constraints on Quasar Lifetime and Obscuration
- The evolution of the Lyman-alpha forest effective optical depth following HeII reionisation
- The VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5<z<5.5 and the colour selection of high redshift galaxies
- Mapping quasar light echoes in 3D with Lyα forest tomography
- Measuring the Density Fields around Bright Quasars at with XQR-30 Spectra
- Dating individual quasars with the HeII proximity effect
- Constraints on ionising photon production from the large-scale Lyman-alpha forest
- Constraining the Contribution of Galaxies and Active Galactic Nuclei to Cosmic Reionization
- Constraining the Gravitational Lensing of Quasars from their Proximity Zones
- The First Gamma-ray Emitting BL Lacertae Object at the Cosmic Dawn
- A Novel Statistical Method for Measuring the Temperature-Density Relation in the IGM Using the - Distribution of Absorbers in the Ly Forest
- Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations
- Probing the environment of high-z quasars using the proximity effect in projected quasar pairs
- The ESO UVES Advanced Data Products Quasar Sample - IV. On the deficiency of Argon in DLA systems
- Joint Bayesian Estimation of Quasar Continua and the Lyman-Alpha Forest Flux Probability Distribution Function
- The association between gas and galaxies III: The Cross-correlation of Galaxies and Ly-alpha Absorbers at z ~ 1
- On probing the properties of QSOs through their proximity effects on the intergalactic medium
- The Circumgalactic Medium in Massive Halos
- High-ion absorption in the proximate damped Lyman-alpha system toward Q0841+129
- Log-Poisson Non-Gaussianity of Ly Transmitted Flux Fluctuations at High Redshift
- The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS
- Cosmological radiative transfer for the line-of-sight proximity effect
- Effective Opacity of the Intergalactic Medium from Galaxy Spectra Analysis
- Probing Large Scale Ionizing Background Fluctuation with Lyman Forest and Galaxy Cross-correlation at z=2.4
- Fluctuations of the intergalactic ionization field at redshift z ~ 2
- Analysis of methods for detecting the proximity effect in quasar spectra
- Large scale environmental bias of the QSO line of sight proximity effect
- Spectral Signatures of Quasar Ages at z~3
- Constraining the ratio of median pixel optical depth profile around z ~ 4 quasars using the longitudinal proximity effect
- Redshift determination through weighted phase correlation: a linearithmic implementation
- QUEST (Quasar Unsupervised Encoder and Synthesis Tool): A machine learning framework to generate quasar spectra
- Measurements of quasar proximity zones with the Ly forest of DESI Y1 quasars