MMT Spectroscopy of Lyman-alpha at z7: Evidence for Accelerated Reionization Around Massive Galaxies
arXiv:2010.03566 · doi:10.1093/mnras/stab432
Abstract
Reionization-era galaxies tend to exhibit weak Ly emission, likely reflecting attenuation from an increasingly neutral IGM. Recent observations have begun to reveal exceptions to this picture, with strong Ly emission now known in four of the most massive z=79 galaxies in the CANDELS fields, all of which also exhibit intense [OIII]H emission (EW800 ). To better understand why Ly is anonymously strong in a subset of massive z79 galaxies, we have initiated an MMT/Binospec survey targeting a larger sample (N=22) of similarly luminous (16 L) z7 galaxies selected over very wide-area fields (3 deg). We confidently (7) detect Ly in 78% (7/9) of galaxies with strong [OIII]H emission (EW800 ) as opposed to only 8% (1/12) of galaxies with more moderate (EW=200800 ) [OIII]H. We argue that the higher Ly EWs of the strong [OIII]H population likely reflect enhanced ionizing photon production efficiency owing to their large sSFRs (30 Gyr). We also find evidence that Ly transmission from massive galaxies declines less rapidly over than in low-mass lensed systems. In particular, our data suggest no strong evolution in Ly transmission, consistent with a picture wherein massive z7 galaxies often reside in large ionized regions. We detect three closely-separated ( = 1.7 physical Mpc) z7 Ly emitters in our sample, conceivably tracing a large ionized structure that is consistent with this picture. We detect tentative evidence for an overdensity in this region, implying a large ionizing photon budget in the surrounding volume.
arXiv comment20 pages, 11 figures. Accepted in MNRAS with minor revisions
References in corpus (155)
- Astropy: A Community Python Package for Astronomy
- The NumPy array: a structure for efficient numerical computation
- Stellar population synthesis at the resolution of 2003
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics
- Rest-Frame Ultraviolet Spectra of z~3 Lyman Break Galaxies
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5
- The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
- Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and Hubble Space Telescope
- UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
- Observational constraints on Cosmic Reionization
- The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years
- The Pan-STARRS1 Surveys
- Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models
- The Growth of HII Regions During Reionization
- The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN
- New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign
- Model-independent evidence in favor of an end to reionization by z~6
- Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program
- The Abundance of Star-Forming Galaxies in the Redshift Range 8.5 to 12: New Results from the 2012 Hubble Ultra Deep Field Campaign
- COSMOS : Hubble Space Telescope Observations
- An updated analytic model for the attenuation by the intergalactic medium
- Efficient Simulations of Early Structure Formation and Reionization
- The 2013 Release of Cloudy
- Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies: - I. New constraints on cosmic reionisation from the luminosity and redshift-dependent fraction of Lyman-alpha emission
- The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8
- Reionization after Planck: The Derived Growth of the Cosmic Ionizing Emissivity now matches the Growth of the Galaxy UV Luminosity Density
- Evidence of patchy hydrogen reionization from an extreme Ly trough below redshift six
- Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
- UV-Continuum Slopes of >4000 z~4-8 Galaxies from the HUDF/XDF, HUDF09, ERS, CANDELS-South, and CANDELS-North Fields
- A new multi-field determination of the galaxy luminosity function at z=7-9 incorporating the 2012 Hubble Ultra Deep Field imaging
- The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr
- Spectroscopic Confirmation of Three z-Dropout Galaxies at z = 6.844 - 7.213: Demographics of Lyman-Alpha Emission in z ~ 7 Galaxies
- Reionization of the Intergalactic Medium and the Damping Wing of the Gunn-Peterson Trough
- Directly Observing the Galaxies Likely Responsible for Reionization
- The Universe is Reionizing at z~7: Bayesian Inference of the IGM Neutral Fraction Using Ly Emission from Galaxies
- Cosmic Reionization after Planck: Could Quasars Do It All?
- Lyman-alpha and CIII] Emission in z=7-9 Galaxies: Accelerated Reionization Around Luminous Star Forming Systems?
- The morphology of HII regions during reionization
- The VISTA Deep Extragalactic Observations (VIDEO) Survey
- The Reionization of the Universe by the First Stars and Quasars
- Luminosity functions of Lyman-alpha emitters at z=6.5, and z=5.7: evidence against reionization at z=6
- Modelling the nebular emission from primeval to present-day star-forming galaxies
- The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift
- Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7
- Evidence for Ubiquitous, High-EW Nebular Emission in z~7 Galaxies: Towards a Clean Measurement of the Specific Star Formation Rate using a Sample of Bright, Magnified Galaxies
- Rapid Reionization by the Oligarchs: The Case for Massive, UV-Bright, Star-Forming Galaxies with High Escape Fractions
- Spectroscopic confirmation of z~7 LBGs: probing the earliest galaxies and the epoch of reionization
- Lyman Alpha Emitting Galaxies as a Probe of Reionization
- The Spectral Energy Distributions Of z~8 Galaxies From The IRAC Ultra Deep Fields: Emission Lines, Stellar Masses, And Specific Star Formation Rates At 650 Myr
- Keck Spectroscopy of Faint 3<z<8 Lyman Break Galaxies:- Evidence for a Declining Fraction of Emission Line Sources In the Redshift Range 6<z<8
- Line Emitting Galaxies Beyond a Redshift of 7: An Improved Method for Estimating the Evolving Neutrality of the Intergalactic Medium
- New observations of z~7 galaxies: evidence for a patchy reionization
- A Rapidly Star-forming Galaxy 700 Million Years After the Big Bang at z=7.51
- Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies:- II. A High Fraction of Line Emitters at Redshift Six
- Large Lyman-alpha opacity fluctuations and low CMB tau in models of late reionization with large islands of neutral hydrogen extending to z<5.5
- Lyman-alpha Emission from a Luminous z=8.68 Galaxy: Implications for Galaxies as Tracers of Cosmic Reionization
- Inferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey
- Completing the Census of Ly-alpha Emitters at the Reionization Epoch
- A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z=7.730 using Keck/MOSFIRE
- Planck intermediate results. XLVII. Planck constraints on reionization history
- Detection of an oxygen emission line from a high redshift galaxy in the reionization epoch
- Probing reionization with Lyman-alpha emission lines
- Z > 7 galaxies with red Spitzer/IRAC [3.6]-[4.5] colors in the full CANDELS data set: the brightest-known galaxies at Z ~ 7-9 and a probable spectroscopic confirmation at Z=7.48
- A lack of evolution in the very bright-end of the galaxy luminosity function from z = 8-10
- Very Strong Emission-Line Galaxies in the WISP Survey and Implications for High-Redshift Galaxies
- Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at Derived with the Half-Million Dropouts on the 100 deg Sky
- Star Formation at From the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH)
- The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?
- An Atlas of z=5.7 and z=6.5 Ly alpha Emitters
- The changing Lya optical depth in the range 6<z<9 from MOSFIRE spectroscopy of Y-dropouts
- Lyman-Alpha-Emitting Galaxies at z = 2.1 in ECDF-S: Building Blocks of Typical Present-day Galaxies?
- Rapid Decline of Lyman-alpha Emission Toward the Reionization Era
- Spectroscopic confirmation of two Lyman break galaxies at redshift beyond 7
- A Significantly Neutral Intergalactic Medium Around the Luminous z=7 Quasar J0252-0503
- Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5
- The Ly-alpha Properties of Faint Galaxies at z2-3 with Systemic Redshifts and Velocity Dispersions from Keck-MOSFIRE
- Simultaneous Multicolor Detection of Faint Galaxies in the Hubble Deep Field
- Long troughs in the Lyman- forest below redshift 6 due to islands of neutral hydrogen
- The Spitzer Extragalactic Representative Volume Survey (SERVS): survey definition and goals
- High-precision Photometric Redshifts from Spitzer/IRAC: Extreme [3.6]-[4.5] Colors Identify Galaxies in the Redshift Range z~6.6-6.9
- MMT/MMIRS spectroscopy of extreme [OIII] emitters: Implications for galaxies in the reionization-era
- Accelerated Evolution of Ly Luminosity Function at Revealed by the Subaru Ultra-Deep Survey for Ly Emitters at
- The Relationship Between Stellar Populations and Lyman Alpha Emission in Lyman Break Galaxies
- Unveiling the nature of bright z ~ 7 galaxies with the Hubble Space Telescope
- Tracing the reionization epoch with ALMA: [CII] emission in z~7 galaxies
- The lack of intense Lyman~alpha in ultradeep spectra of z=7 candidates in GOODS-S: imprint of reionization?
- Are we witnessing the epoch of reionisation at from the spectrum of J1120+0641?
- First Results from the Lyman Alpha Galaxies in the Epoch of Reionization (LAGER) Survey: Cosmological Reionization at z ~ 7
- Star formation and the interstellar medium in z>6 UV-luminous Lyman-break galaxies
- The [OIII]H Equivalent Width Distribution at z7: Implications for the Contribution of Galaxies to Reionization
- Spectroscopy of z ~ 7 candidate galaxies: Using Lyman-alpha to constrain the neutral fraction of hydrogen in the high-redshift universe
- The First Systematic Survey for Lyman Alpha Emitters at z=7.3 with Red-sensitive Subaru/Suprime-Cam
- Quasar Strömgren Spheres Before Cosmological Reionization
- Evolution of the Sizes of Galaxies over 7<z<12 Revealed by the 2012 Hubble Ultra Deep Field Campaign
- Observational Searches for Galaxies at z > 6
- SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7
- No missing photons for reionization: moderate ionizing photon escape fractions from the FIRE-2 simulations
- The GREATS H+[OIII] Luminosity Function and Galaxy Properties at : Walking the Way of JWST
- Gas Clumping in Self-Consistent Reionisation Models
- Binospec: A Wide-field Imaging Spectrograph for the MMT
- CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch
- A spectroscopic search for AGN activity in the reionization era
- Observing the tail of reionization: neutral islands in the Lyman- Forest
- New Insights on Ly-alpha and Lyman Continuum Radiative Transfer in the Greenest Peas
- The Brightest Galaxies over the COSMOS UltraVISTA Field
- The origin of the escape of Lyman alpha and ionizing photons in Lyman Continuum Emitters
- The Global History of Reionisation
- Galactic porosity and a star formation threshold for the escape of ionising radiation from galaxies
- Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
- The Star Formation Demographics of Galaxies in the Local Volume
- Lyman-alpha Emitters During the Early Stages of Reionization
- Physical properties and H-ionizing-photon production rates of extreme nearby star-forming regions
- Beacons into the Cosmic Dark Ages: Boosted transmission of Ly from UV bright galaxies at
- The Rest-Frame Optical Spectroscopic Properties of Ly-Emitters at : The Physical Origins of Strong Ly Emission
- Measurement of Galaxy Clustering at z~7.2 and the Evolution of Galaxy Bias from 3.8<z<8 in the XDF, GOODS-S AND GOODS-N
- Inferences on the distribution of Ly-alpha emission of z~7 and z~8 galaxies
- Non-parametric analysis of the rest-frame UV sizes and morphological disturbance amongst L* galaxies at 4<z<8
- Onset of Cosmic Reionization: Evidence of An Ionized Bubble Merely 680 Myrs after the Big Bang
- Measuring the properties of reionised bubbles with resolved Lyman alpha spectra
- A VLT/FORS2 view at : Lyman- emitter fraction and galaxy physical properties at the edge of the epoch of cosmic reionization
- The physical properties of Lyalpha emitting galaxies: not just primeval galaxies?
- Spectroscopic Constraints on UV Metal Line Emission at z~6-9: The Nature of Lyman-alpha Emitting Galaxies in the Reionization-Era
- The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly Visibility During the Epoch of Reionization
- A New Constraint on Reionization from Evolution of the Ly Luminosity Function at Probed by a Deep Census of Ly Emitter Candidates to 0.3
- Spitzer Matching survey of the UltraVISTA ultra-deep Stripes (SMUVS): Full-mission IRAC Mosaics and Catalogs
- Newly Discovered Bright z~9-10 Galaxies and Improved Constraints on Their Prevalence Using the Full CANDELS Area
- First observational support for overlapping reionized bubbles generated by a galaxy overdensity
- Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
- Hydrodynamic Response of the Intergalactic Medium to Reionization
- The Distribution of Bubble Sizes During Reionization
- Undetected Sources Allow Transmission of the Lyman-alpha Line From Galaxies Prior to Reionization
- Lyman-alpha emitters gone missing: the different evolution of the bright and faint populations
- Spectroscopic investigation of a reionized galaxy overdensity at z=7
- A New Constraint on the Ly Fraction of UV Very Bright Galaxies at Redshift 7
- The Hydrodynamic Feedback of Cosmic Reionization on Small-Scale Structures and Its Impact on Photon Consumption during the Epoch of Reionization
- Keck/MOSFIRE Spectroscopy of z=7-8 Galaxies: Ly Emission from a Galaxy at z=7.66
- First results from Faint Infrared Grism Survey (FIGS): first simultaneous detection of Lyman-alpha emission and Lyman break from a galaxy at z=7.51
- Probing the Reionization History Using the Spectra of High-Redshift Sources
- Binospec Software System
- The VIMOS Ultra Deep Survey: Ly Emission and Stellar Populations of Star-Forming Galaxies at 2<z<2.5
- HST imaging of the brightest z~8-9 galaxies from UltraVISTA: the extreme bright end of the UV luminosity function
- Spectroscopically Confirmed Lyman-Alpha Emitters from Redshift 5 to 7 Behind Ten Galaxy Cluster Lenses
- First Spectroscopic Confirmations of z ~ 7.0 Lya Emitting Galaxies in the LAGER Survey
- Optical Line Emission from z6.8 Sources with Deep Constraints on Ly Visibility
- On the AGN nature of two UV bright sources at z_spec~5.5 in the CANDELS fields: an update of the AGN space density at M1450~-22.5
- Extreme emission-line galaxies out to z1 in zCOSMOS. I. Sample and characterization of global properties
- The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy
- Discovery of a z = 7.452 High Equivalent Width Lyman-α Emitter from the Hubble Space Telescope Faint Infrared Grism Survey
- Texas Spectroscopic Search for Ly Emission at the End of Reionization I. Constraining the Ly Equivalent Width Distribution at 6.0 < < 7.0
- Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionised bubble at z = 6.53
- Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
- The SpeX Prism Library: 1000+ Low-resolution, Near-infrared Spectra of Ultracool M, L, T and Y Dwarfs
Cited by in corpus (52)
- Galaxy Formation and Reionization: Key Unknowns and Expected Breakthroughs by the James Webb Space Telescope
- Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe
- The Low-Redshift Lyman Continuum Survey II: New Insights into LyC Diagnostics
- New Insights into the Evolution of Massive Stars and Their Effects on Our Understanding of Early Galaxies
- Star formation histories of UV-luminous galaxies at : implications for stellar mass assembly at early cosmic times
- The THESAN project: Lyman-alpha emission and transmission during the Epoch of Reionization
- First Sample of H+[O III] 5007 Line Emitters at Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line Luminosity Functions
- Searching for Islands of Reionization: A Potential Ionized Bubble Powered by a Spectroscopic Overdensity at z = 8.7
- Inferring the IGM Neutral Fraction at z ~ 6-8 with Low-Luminosity Lyman Break Galaxies
- A short mean free path at favors late and rapid reionization by faint galaxies
- Strong Ly Emission in an Overdense Region at : A Very Large ( physical Mpc) Ionized Bubble in COSMOS?
- ALMA Confirmation of an Obscured Hyperluminous Radio-Loud AGN at Associated with a Dusty Starburst in the 1.5 deg COSMOS Field
- Early Results from GLASS-JWST. I: Confirmation of Lensed Lyman-Break Galaxies Behind the Abell 2744 Cluster With NIRISS
- High Equivalent Width of Hα+[N II] Emission in z~8 Lyman-break Galaxies from IRAC 5.8μm Observations: Evidence for Efficient Lyman-continuum Photon production in the Epoch of Re-ionization
- Dusty winds clear JWST super-early galaxies
- The ALMA REBELS Survey: Efficient Ly Transmission of UV-Bright z7 Galaxies from Large Velocity Offsets and Broad Line Widths
- Lyman-alpha spectroscopy of extreme [OIII] emitting galaxies at : Implications for Ly visibility and LyC leakage at
- The Prevalence of Galaxy Overdensities Around UV-Luminous Lyman Emitters in the Epoch of Reionization
- Equivalent widths of Lyman emitters in MUSE-Wide and MUSE-Deep
- JADES: Primaeval Lyman- emitting galaxies reveal early sites of reionisation out to redshift
- First Peek with JWST/NIRCam Wide-Field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O III]/H Emitter at
- Crucial Factors for Lyα Transmission in the Reionizing Intergalactic Medium: Infall Motion, HII Bubble Size, and Self-shielded Systems
- Dark-ages Reionization and Galaxy Formation Simulation XX. The Ly IGM transmission properties and environment of bright galaxies during the Epoch of Reionization
- Radio and Far-IR Emission Associated with a Massive Star-forming Galaxy Candidate at z6.8: A Radio-Loud AGN in the Reionization Era?
- The ionizing photon production efficiency of bright z2-5 galaxies
- The Morphology of Reionization in a Dynamically Clumpy Universe
- CLEAR: Boosted Ly Transmission of the Intergalactic Medium in UV bright Galaxies
- Constraining Reionization in Progress at z=5.7 with Lyman- Emitters: Voids, Peaks, and Cosmic Variance
- Nature and Nurture? Comparing Ly Detections in UV-Bright and Fainter [O III]+H Emitters at With Keck/MOSFIRE
- First Light And Reionisation Epoch Simulations (FLARES) XIII: The Lyman-continuum emission of high-redshift galaxies
- Illuminating the Dark Side of Cosmic Star Formation III: Building the largest homogeneous sample of Radio-Selected Dusty Star-Forming Galaxies in COSMOS with PhoEBO
- Late-end reionization with ATON-HE: towards constraints from Lyman- emitters observed with JWST
- The THESAN project: Lyman-alpha emitter luminosity function calibration
- Lyman-alpha Emitters in Ionized Bubbles: Constraining the Environment and Ionized Fraction
- Deep Spitzer/IRAC Data for z~10 galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ~500 Myr of Cosmic Time
- Spectroscopic confirmation of a gravitationally lensed Lyman break galaxy at z = 6.827 using NOEMA
- A Framework for Simultaneously Measuring Field Densities and the High-z Luminosity Function
- Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
- 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
- Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly emitters and IGM transmission in the COSMOS field at
- Spectroscopy of an extreme [OIII] emitting active galactic nucleus at : implications for the reionisation era
- Probing Patchy Reionization with the Void Probability Function of Lyman- Emitters
- Subaru/HSC z-Broadband Excess Selection of Extreme Emission Line Galaxies at z<1
- Scattering of Lyα Photons through the Reionizing Intergalactic Medium: I. Spectral Energy Distribution
- Ly Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly detection
- REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization
- Reionization in Protocluster Environments at with JWST/NIRSpec
- Deep JWST spectroscopy of galaxies in a candidate ionized bubble at : probing reionization at pMpc scales with Ly emission
- Exploration of the high-redshift universe enabled by THESEUS
- Constraints on the Epoch of Reionization with Roman Space Telescope and the Void Probability Function of Lyman-Alpha Emitters
- A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
- Euclid: Discovery of bright Lyman-break galaxies in UltraVISTA and Euclid COSMOS