The Keck Lyman Continuum Spectroscopic Survey (KLCS): The Emergent Ionizing Spectrum of Galaxies at
arXiv:1805.06071 · doi:10.3847/1538-4357/aaed28
Abstract
We present results of a deep spectroscopic survey designed to quantify the statistics of the escape of ionizing photons from star-forming galaxies at z~3. We measure the ratio of ionizing to non-ionizing UV flux density <f900/f1500>_obs, where f900 is the mean flux density evaluated over the range [880,910] A. We quantify the emergent ratio of ionizing to non-ionizing UV flux density by analyzing high-S/N composite spectra formed from sub-samples with common observed properties and numbers sufficient to reduce the statistical uncertainty in the modeled IGM+CGM correction to obtain precise values of <f900/f1500>_out, including a full-sample average <f900/f1500>_out=. We further show that <f900/f1500>_out increases monotonically with Ly rest equivalent width, inducing an inverse correlation with UV luminosity as a by-product. We fit the composite spectra using stellar spectral synthesis together with models of the ISM in which a fraction f_c of the stellar continuum is covered by gas with column density N(HI). We show that the composite spectra simultaneously constrain the intrinsic properties of the stars (L900/L1500)_int along with f_c, N(HI), E(B-V), and , the absolute escape fraction of ionizing photons. We find a sample-averaged , and that subsamples fall along a linear relation . We use the FUV luminosity function, the distribution function , and the relationship between and <f900/f1500>_out to estimate the total ionizing emissivity of star-forming galaxies with Muv < -19.5: ergs/s/Hz/Mpc, exceeding the contribution of QSOs by a factor of , and accounting for % of the total at estimated using indirect methods.
arXiv comment45 pages, 31 figures, ApJ, in press
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- Probing Large Scale Ionizing Background Fluctuation with Lyman Forest and Galaxy Cross-correlation at z=2.4
- Towards unveiling the Cosmic Reionization: the ionizing photon production efficiency () of Low-mass H emitters at
- Detections of [C II] 158 m and [O III] 88 m in a Local Lyman Continuum Emitter, Mrk 54, and its Implications to High-redshift ALMA Studies
- Inferring the Distribution of the Ionising Photon Escape Fraction
- A public grid of radiative transfer simulations for Lyman-alpha and metal lines in idealised galactic outflows
- ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
- The Importance of Dust Distribution in Ionizing-photon Escape: NIRCam and MIRI Imaging of a Lyman Continuum-emitting Galaxy at z ~ 3.8
- The Lyman-alpha and Continuum Origins Survey II: the connection between the escape of ionizing radiation and Lyman-alpha halos in star-forming galaxies
- A Simulated Galaxy Laboratory: Exploring the Observational Effects on UV Spectral Absorption Line Measurements
- Euclid preparation. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
- The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions
- The Role of Dust, UV Luminosity and Large-scale Environment on the Escape of Lya Photons: A Case Study of a Protocluster field at z = 3.1
- Does radiative feedback make faint z>6 galaxies look small?
- The Ly and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties and LyC Escape
- Clues to the nature of dark matter from first galaxies
- Lyman-alpha at Cosmic Noon I: Ly-alpha Spectral Type Selection of z ~ 2-3 Lyman Break Galaxies with Broadband Imaging
- Emission Line Galaxies in the SHARDS Hubble Frontier Fields II: Limits on Lyman-Continuum Escape Fractions of Lensed Emission Line Galaxies at Redshifts 2 < z < 3.5
- KBSS-InCLOSE I: Design and First Results from the Inner CGM of QSO Line Of Sight Emitting Galaxies at z~2-3
- SDSS-IV MaNGA: an observational evidence of density bounded region in a Lyman- emitter
- The Lyman Alpha Reference Sample. XVI. Global 21cm HI properties of Lyman- emitting galaxies
- The impact of cosmic ray feedback during the epoch of reionisation
- Gamma-Ray Absorption By The Cosmic Lyman Continuum From Star-forming Galaxies
- Discovery of a damped Ly galaxy at z 3 towards the quasar SDSS J011852+040644
- CECILIA: Ultra-Deep Rest-Optical Spectra of Faint Galaxies at Cosmic Noon
- Exploration of the high-redshift universe enabled by THESEUS
- Power-law Emission-line Wings and Radiation-Driven Superwinds in Local Lyman Continuum Emitters
- Lyman-alpha at Cosmic Noon II: The relationship between kinematics and Lyman-alpha in z~2-3 Lyman Break Galaxies
- A Lyman continuum analysis for galaxies at in the Abell 2744 Cluster Field
- Constraining cosmic ray transport models using circumgalactic medium properties and observables
- Unraveling the Lyman Continuum Emission of Ion3: Insights from HST multi-band imaging and X-Shooter spectroscopy
- A resolved Lyman-Alpha profile with doubly peaked emission at z~7
- The Parallel Ionizing Emissivity Survey (PIE). I. Survey design and selection of candidate Lyman Continuum leakers at 3.1<z<3.5
- The CUBES Science Case
- The JWST early galaxy crisis resolved by a reionization degeneracy
- Nitrogen abundances in star-forming galaxies 2.2 Gyr after the Big Bang are not elevated