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
arXiv:0707.3161 · doi:10.1086/527673
Abstract
We present luminosity functions (LFs) and various properties of Lya emitters (LAEs) at z=3.1, 3.7, and 5.7, in a 1 deg^2 sky of the Subaru/XMM-Newton Deep Survey (SXDS) Field. We obtain a photometric sample of 858 LAE candidates based on deep Subaru/Suprime-Cam imaging data, and a spectroscopic sample of 84 confirmed LAEs from Subaru/FOCAS and VLT/VIMOS spectroscopy in a survey volume of ~10^6 Mpc^3 with a limiting Lya luminosity of ~3x10^42 erg/s. We derive the LFs of Lya and UV-continuum (~1500 Å) for each redshift, taking into account the statistical error and the field-to-field variation. We find that the apparent Lya LF shows no significant evolution between z=3.1 and 5.7 within factors of 1.8 and 2.7 in L* and phi*, respectively. On the other hand, the UV LF of LAEs increases from z=3.1 to 5.7, indicating that galaxies with Lya emission are more common at earlier epochs. We identify six LAEs with AGN activities from our spectra combined with VLA, Spitzer, and XMM-Newton data. Among the photometrically selected LAEs at z=3.1 and 3.7, only ~1 % show AGN activities, while the brightest LAEs with logL(Lya) >~ 43.4-43.6 erg/s appear to always host AGNs. Our LAEs are bluer in UV-continuum color than dropout galaxies, suggesting lower extinction and/or younger stellar populations. Our stacking analyses provide upper limits to the radio luminosity and the f(HeII)/f(Lya) line fraction, and constrain the hidden star formation (+low-luminosity AGN) and the primordial population in LAEs.
arXiv comment75 pages, 27 figures; ApJS in press. High resolution version at http://www.ociw.edu/~ouchi/work/astroph/sxds_LAEs/ouchi_SXDSLAE_ApJS.pdf
References in corpus (108)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Stellar population synthesis at the resolution of 2003
- The Dust Content and Opacity of Actively Star-Forming Galaxies
- The Global Schmidt Law in Star Forming Galaxies
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- The Formation of Galactic Disks
- Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
- Lyman Break Galaxies at z>4 and the Evolution of the UV Luminosity Density at High Redshift
- Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z ~ 6 Quasars II: A Sample of 19 Quasars
- Rest-Frame Ultraviolet Spectra of z~3 Lyman Break Galaxies
- The Star Formation History of Field Galaxies
- The Hubble Ultra Deep Field
- The Dust Opacity of Star-Forming Galaxies
- SWIRE: The SIRTF Wide-area InfraRed Extragalactic Survey
- Subaru Prime Focus Camera -- Suprime-Cam --
- Lyman Break Galaxies at Redshift z~3: Survey Description and Full Data Set
- The 2dF QSO Redshift Survey - XII. The spectroscopic catalogue and luminosity function
- Lyman Alpha Imaging of a Proto-Cluster Region at <z>=3.09
- The Rest-Frame Extreme Ultraviolet Spectral Properties of QSOs
- The transition from Population III to normal galaxies: Ly-a and HeII 1640 emission and the ionising properties of high redshift starburst galaxies
- Subaru Deep Survey V. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Photometric Properties
- The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- II. Submillimetre maps, catalogue and number counts
- The End of the Reionization Epoch Probed by Ly-alpha Emitters at z=6.5 in the Subaru Deep Field
- High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data IV: Luminosity Function from the Fall Equatorial Stripe Sampl
- Red and Reddened Quasars in the Sloan Digital Sky Survey
- A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey III: Discovery of Five Additional Quasars
- Ly-alpha Emission-Line Galaxies at z = 3.1 in the Extended Chandra Deep Field South
- Galaxies at z~6: The UV Luminosity Function and Luminosity Density from 506 UDF, UDF-Ps, and GOODS i-dropouts
- Luminosity functions of Lyman-alpha emitters at z=6.5, and z=5.7: evidence against reionization at z=6
- The SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies
- A Subaru Search for Ly-alpha Blobs in and around the Proto-cluster Region at Redshift z=3.1
- High-z Lyman-alpha Emitters. I. A Blank-Field Search for Objects Near Redshift z=3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA22
- A galaxy at a redshift z = 6.96
- Large Equivalent width Lyman-alpha line emission at z=4.5: young galaxies in a young universe
- Ly Alpha Emitters at z=5.7 in the Subaru Deep Field
- A Redshift z = 6.56 Galaxy Behind the Cluster Abell 370
- The Star Formation Rate of the Universe at z~6 from the Hubble Ultra Deep Field
- Subaru Deep Survey II. Luminosity Functions and Clustering Properties of Lya Emitters at z=4.86 in the Subaru Deep Field
- The Subaru Deep Field Project: Lyman Emitters at Redshift of 6.6
- The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6
- The Luminosity Function of Lyman Alpha Emitters at Redshift z~5.7
- Spectroscopic Identification of Massive Galaxies at z~2.3 with Strongly Suppressed Star Formation
- Spectroscopic Confirmation of Three Redshift 5.7 Lyman-alpha Emitters from the Large Area Lyman Alpha Survey
- Protoclusters associated with z > 2 radio galaxies. I. Characteristics of high redshift protoclusters
- Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source population
- The Detectability of the First Stars and Their Cluster Enrichment Signatures
- The Great Observatories Origins Deep Survey VLT/FORS2 Spectroscopy in the GOODS-South Field: Part II
- The Discovery of Two Lyman Emitters Beyond Redshift 6 in the Subaru Deep Field
- Subaru Deep Survey VI. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Clustering Properties
- The Physical Nature of Lyman Alpha Emitting Galaxies at z=3.1
- An Explanation for the Observed Weak Size Evolution of Disk Galaxies
- The Space Density and Colors of Massive Galaxies at 2<z<3: the Predominance of Distant Red Galaxies
- Discovery of 9 Ly alpha emitters at redshift z~3.1 using narrow-band imaging and VLT spectroscopy
- A Keck Survey for Gravitationally-Lensed Lyman-alpha Emitters in the Redshift Range 8.5 < z < 10.4: New Constraints on the Contribution of Low Luminosity Sources to Cosmic Reionization
- Current Performance and On-Going Improvements of the 8.2 m Subaru Telescope
- Candidates of z ~ 5.5--7 Galaxies in the HST Ultra Deep Field
- Optical to mid-IR observations of Lyman-alpha galaxies at redshift 5 in the HUDF: a young and low mass population
- The Population of Faint Optically-Selected AGN at z~3
- A Faint Star-Forming System Viewed Through the Lensing Cluster Abell 2218: First Light at z~5.6?
- Lyman Alpha Emitters at Redshift z=5.7
- Discovery of a Large ~200 kpc Gaseous Nebula at z=2.7 with the Spitzer Space Telescope
- A Lyman-alpha blob in the GOODS South field: evidence for cold accretion onto a dark matter halo
- Keck Deep Fields. II. The UV Galaxy Luminosity Function at z~4, 3, and 2
- Colour corrections for high redshift objects due to intergalactic attenuation
- An overdensity of galaxies at z=5.9 +/-0.2 in the Ultra Deep Field confirmed using the ACS grism
- Spectroscopic Properties of the z=4.5 Lyman-alpha Emitters
- HST imaging and Keck Spectroscopy of z~6 I-band Drop-Out Galaxies in the ACS GOODS Fields
- Subaru Deep Survey. IV. Discovery of a Large-Scale Structure at Redshift \simeq 5
- The Abundance of Low-luminosity Lyman alpha Emitters at High Redshift
- A multi-wavelength study of z = 3.15 Lyman-alpha emitters in the GOODS South Field
- The Ages and Masses of Lyman Alpha Galaxies at Redshift
- Luminous Lyman Break Galaxies at z>5 and the Source of Reionization
- Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field
- A Subaru Search for Lyman Emitters at Redshift 5.7
- Deficiency of large equivalent width Lyman-alpha emission in luminous Lyman break galaxies at z~5-6?
- Significant primordial star formation at redshifts z ~ 3-4
- Three Lyman-alpha Emitters at z approx 6: Early GMOS/Gemini Data from the GLARE Project
- Number Density of Bright Lyman-Break Galaxies at z~6 in the Subaru Deep Field
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- The Stellar Population of Lyman-alpha Emitting Galaxies at z ~ 5.7
- Systematic Survey of Extended Lyman-alpha Sources over z~3-5
- Spitzer Constraints on the z=6.56 Galaxy Lensed by Abell 370
- The GLARE Survey II. Faint z=6 Ly-alpha Line Emitters in the HUDF
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- Spectroscopy of z~6 i-dropout Galaxies: Frequency of Ly-alpha Emission and the Sizes of Ly-alpha Emitting Galaxies
- The Number Density of Old Passively-Evolving Galaxies at z=1 in the Subaru/XMM-Newton Deep Survey Field
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- Constraints to the evolution of Ly-Alpha bright galaxies between z=3 and z=6
- The Space Density of Redshift 5.7 Ly-Alpha Emitters
- Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release
- A VLT/FORS2 Multi-Slit Search for Lyman-alpha Emitting Galaxies at z~6.5
- The Subaru/XMM-Newton Deep Survey (SXDS) - V. Optically Faint Variable Object Survey
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- A Subaru Search for Lyman-Alpha Emitters at z=5.8 with an Intermediate-Band Filter
- Narrow-Band Survey of the GOODS Fields: Search for Lyman-Alpha Emitters at z = 5.7
- The Wide Field Imager Lyman-Alpha Search (WFILAS) for Galaxies at Redshift ~5.7: II. Survey Design and Sample Analysis
- The Wide Field Imager Lyman-Alpha Search (WFILAS) for Galaxies at Redshift ~5.7: I. A Spatially Compact Lyman-alpha Emitting Galaxy at Redshift 5.721
- An Intermediate-band imaging survey for high-redshift Lyman Alpha Emitters: The Mahoroba-11
- Radio and millimeter properties of Ly emitters in the COSMOS field: limits on radio AGN, submm galaxies, and dust obscuration
- The VIMOS VLT Deep Survey:The ultraviolet galaxy luminosity function and luminosity density at 3<z<4
- Preliminary Results from a Spectrosopic LyA Survey at Redshift 5.7 with IMACS
- Lyman Break Galaxies in the VLT/FORS2 spectroscopic campaign in the GOODS-S field
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- Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models
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- Diffuse Lyman Alpha Emitting Halos: A Generic Property of High Redshift Star Forming Galaxies
- Lyman-alpha and CIII] Emission in z=7-9 Galaxies: Accelerated Reionization Around Luminous Star Forming Systems?
- Ionization State of Inter-Stellar Medium in Galaxies: Evolution, SFR-M_star-Z Dependence, and Ionizing Photon Escape
- The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6
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- Evidence for PopIII-like stellar populations in the most luminous Lyman- emitters at the epoch of re-ionisation: spectroscopic confirmation
- CANDELS Multiwavelength catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-Deep Survey Field
- The spectral evolution of the first galaxies. I. James Webb Space Telescope detection limits and color criteria for population III galaxies
- Using Lyman-alpha to detect galaxies that leak Lyman continuum
- Lyman Alpha Emitting Galaxies as a Probe of Reionization
- Large Area Survey for z=7 Galaxies in SDF and GOODS-N: Implications for Galaxy Formation and Cosmic Reionization
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- Keck Spectroscopy of Faint 3<z<7 Lyman Break Galaxies:- II. A High Fraction of Line Emitters at Redshift Six
- Completing the Census of Ly-alpha Emitters at the Reionization Epoch
- Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly
- Hyper-Eddington accretion flows onto massive black holes
- A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems
- Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: Evidence for extremely low metallicities?
- The MUSE 3D view of the Hubble Deep Field South
- Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program Strategy and Clustering Properties of ~2,000 Lya Emitters at z=6-7 over the 0.3-0.5 Gpc Survey Area
- Star formation at z=1.47 from HiZELS: An Hα+[OII] double-blind study
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- 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
- Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.9
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- An Atlas of z=5.7 and z=6.5 Ly alpha Emitters
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- Stellar Populations of Lyman Alpha Emitters at z~6-7: Constraints on the Escape Fraction of Ionizing Photons from Galaxy Building Blocks
- The HETDEX Pilot Survey. II. The Evolution of the Ly-alpha Escape Fraction from the UV Slope and Luminosity Function of 1.9<z<3.8 LAEs
- Identification of the brightest Lyα emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era
- Accelerated Evolution of Ly Luminosity Function at Revealed by the Subaru Ultra-Deep Survey for Ly Emitters at
- The Spectroscopic Properties of Lyα-Emitters at z 2.7: Escaping Gas and Photons from Faint Galaxies
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- The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]-1908Å~emission 10.8 to 12.5 Gyr ago
- On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6
- No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman- emitter 'CR7'
- Can galactic outflows explain the properties of Ly-alpha emitters?
- The Ly Luminosity Function and Cosmic Reionization at 7.0: a Tale of Two LAGER Fields
- Large-scale clustering of Lyman-alpha emission intensity from SDSS/BOSS
- Three Lyman-alpha emitting galaxies within a quasar proximity zone at z=5.8
- Confirmation of a Steep Luminosity Function for Lyman-alpha Emitters at z = 5.7: A Major Component of Reionization
- The UV, Lyman-alpha, and dark matter halo properties of high redshift galaxies
- Discovery of a Very Large Structure at Z=3.78
- An Empirical Study of the Relationship between Lyα and UV selected Galaxies: Do Theorists and Observers `Select' the Same Objects?
- A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?
- Lyman-alpha emitters gone missing: the different evolution of the bright and faint populations
- CHORUS II. Subaru/HSC Determination of the Ly Luminosity Function at : Constraints on Cosmic Reionization Model Parameter
- Spectroscopic Confirmation of a Protocluster at z=3.786
- On the influence of physical galaxy properties on Lyman-alpha escape in star-forming galaxies
- The clustering of Ly-alpha emitters in a LambdaCDM Universe
- Intensity mapping with SDSS/BOSS Lyman-alpha emission, quasars and their Lyman-alpha forest
- Modelling the observed luminosity function and clustering evolution of Lyman- emitters: growing evidence for late reionization
- What is the Physical Origin of Strong Lya Emission? I. Demographics of Lya Emitter Structures
- MUSE Deep-Fields: The Lya Luminosity Function in the Hubble Deep Field South at 2.91 < z < 6.64
- Large Scale Environment of a Luminous Quasar Probed by Ly Emitters and Lyman Break Galaxies
- Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lyman-alpha Emitters in COSMOS and GOODS-N
- Searching for Neutral Hydrogen Halos around z ~ 2.1 and z ~ 3.1 Ly-alpha Emitting Galaxies
- Limits on the luminosity function of Ly-alpha emitters at z = 7.7
- Lyman Alpha Emitters in Hierarchical Galaxy Formation II. UV Continuum Luminosity Function and Equivalent Width Distribution
- Photometric properties of Ly alpha emitters at z=4.86 in the COSMOS 2 square degree field
- Spectroscopic observation of Ly emitters at z~7.7 and implications on re-ionization
- Evolution of the observed Ly-alpha luminosity function from z = 6.5 to z = 7.7: evidence for the epoch of reionization ?
- On the Diffuse Lyman-alpha Halo Around Lyman-alpha Emitting Galaxies
- Lyman Alpha Driven Outflows Around Star Forming Galaxies
- The escape of ionizing photons from supernova-dominated primordial galaxies
- Anisotropic Lyman-alpha Emission
- The UV-brightest Lyman continuum emitting star-forming galaxy
- Spectroscopy of luminous z>7 galaxy candidates and sources of contamination in z>7 galaxy searches
- The cool side of Lyman Alpha Emitters
- SPLASH-SXDF Multi-wavelength Photometric Catalog
- Bright Strongly Lensed Galaxies at Redshift z~ 6-7 behind the Clusters Abell 1703 and CL0024+161
- The Formation of the massive galaxies in the SSA22 z=3.1 protocluster
- Gemini GMOS spectroscopy of HeII nebulae in M33
- Modelling high redshift Lyman-alpha Emitters
- Serendipitous Discovery of an Overdensity of Lyman-Alpha Emitters at z~4.8 in the Cl1604 Supercluster Field
- The evolution of rest-frame UV properties, Lya EWs and the SFR-Stellar mass relation at z~2-6 for SC4K LAEs
- SILVERRUSH. II. First Catalogs and Properties of ~2,000 Lya Emitters and Blobs at z~6-7 Identified over the 14-21 deg2 Sky
- HETDEX Public Source Catalog 1: 220K Sources Including Over 50K Lyman Alpha Emitters from an Untargeted Wide-area Spectroscopic Survey
- The nature of z ~ 2.3 Lyman-alpha emitters
- The Spectrally Resolved Lyman-alpha Emission of Three Lyman-alpha Selected Field Galaxies at z~2.4 from the HETDEX Pilot Survey
- Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at
- Spectral shapes of the Lyman-alpha emission from galaxies: I. blueshifted emission and intrinsic invariance with redshift
- Lyman-Alpha Emitting Galaxies as a Probe of Reionization: Large-Scale Bubble Morphology and Small-Scale Absorbers
- The UV and Ly Luminosity Functions of galaxies and the Star Formation Rate Density at the end of HI reionization from the VIMOS Ultra-Deep Survey (VUDS)
- The Lyman alpha reference sample: IV. Morphology at low and high redshift
- Exploring the nature of the Lyman- emitter CR7
- A 10 deg Lyman- survey at z=8.8 with spectroscopic follow-up: strong constraints on the LF and implications for other surveys
- Constraining dust formation in high-redshift young galaxies
- The MUSE-Wide survey: A measurement of the Ly emitting fraction among galaxies
- Evolution of Star Formation in the UKIDSS Ultra Deep Survey Field - I. Luminosity Functions and Cosmic Star Formation Rate out to z=1.6
- The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population
- Equivalent widths of Lyman emitters in MUSE-Wide and MUSE-Deep
- First Spectroscopic Confirmations of z ~ 7.0 Lya Emitting Galaxies in the LAGER Survey
- The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at
- The Magellan M2FS Spectroscopic Survey of High- Galaxies: Lyα Emitters at and the Evolution of Lyα Luminosity Function over
- Small-scale Intensity Mapping: Extended Ly, H and Continuum emission as a Probe of Halo Star Formation in High-redshift Galaxies
- How Do Galaxies trace a large scale structure?: A case study around a massive protocluster at
- MUSE Spectroscopic Identifications of Ultra-Faint Emission Line Galaxies with M -15
- Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background
- Strong Clustering of Lyman Break Galaxies around Luminous Quasars at z~4
- SILVERRUSH XI: Constraints on the Ly luminosity function and cosmic reionization at with Subaru/Hyper Suprime-Cam
- Searching for z~7.7 Lyman Alpha Emitters in the COSMOS Field with NEWFIRM
- On Lya emission in z~3-6 UV-selected galaxies
- Stellar Masses of Lyman Break Galaxies, Lyman Alpha Emitters and Radio Galaxies in Overdense Regions at z=4-6
- Were progenitors of local L* galaxies Lyman-alpha emitters at high redshift?
- Lyman `bump' galaxies - II. A possible signature of massive extremely metal-poor or metal-free stars in z=3.1 Ly-alpha emitters
- Observing the first galaxies
- A glance at the host galaxy of high-redshift quasars using strong damped Lyman-alpha systems as coronagraphs
- z~1 Lya Emitters I. The Luminosity Function
- Determining the Nature of Late Gunn-Peterson Troughs with Galaxy Surveys
- A High Space Density of Luminous Lyman Alpha Emitters at z~6.5
- Constraining Lyman-alpha spatial offsets at from VANDELS slit spectroscopy
- Faint end of the luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE
- The clustering of typical Ly emitters from : host halo masses depend on Ly and UV luminosities
- Profiles of Lymanα Emission Lines
- A 16 deg survey of emission-line galaxies at z<1.5 in HSC-SSP PDR1
- Connecting Faint End Slopes of the Lyman- emitter and Lyman-break Galaxy Luminosity Functions
- Ly-alpha emitters in the GOODS-S field: a powerful pure nebular SED with N IV] emission at z=5.563
- Lyα Equivalent Width Distribution of Lyα Emitting Galaxies at Redshift z 4.5
- MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063: II. Properties of low luminosity Lyman alpha emitters at z>3
- Constraints on the End of Reionization from the Density Fields Surrounding Two Highly Opaque Quasar Sightlines
- Detecting Lyman Alpha Emitters in the Sub-millimeter
- The Lyman-alpha emission of high-z damped Lyman-alpha systems
- How Lyman Alpha Emission Depends On Galaxy Stellar Mass
- Evolution of Lyman Alpha Galaxies: Stellar Populations at z ~ 0.3
- The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
- Ultra-Luminous X-ray Sources in Haro 11 and the Role of X-ray Binaries in Feedback in Lyman-alpha Emitting Galaxies
- MUSE observations of the lensing cluster Abell 1689
- Ly-alpha emitting galaxies at redshift z~4.5 in the LALA Cetus field
- The Building the Bridge survey for z=3 Ly-alpha emitting galaxies II: Completion of the survey
- Crucial Factors for Lyα Transmission in the Reionizing Intergalactic Medium: Infall Motion, HII Bubble Size, and Self-shielded Systems
- A search for AGN in the most extreme UV-selected starbursts using the European VLBI Network
- J-PLUS: Unveiling the brightest-end of the Lyα luminosity function at 2.0<z<3.3 over 1000 deg^2
- Bright Lyman-alpha Emitters at z~9: constraints on the luminosity function from HiZELS
- Lyman-Alpha Emitter Galaxies at z ~ 2.8 in the Extended Chandra Deep Field-South: I. Tracing the Large-Scale Structure via Lyman-Alpha Imaging
- CLARA's view on the escape fraction of Lyman-Alpha photons in high redshift galaxies
- A Faint Flux-Limited Lyman Alpha Emitter Sample at
- Lyman alpha Luminosity Functions at Redshift z = 4.5
- Effect of Intergalactic Medium on the Observability of Lyman Alpha Emitters during Cosmic Reionization
- A new quadruple gravitational lens from the Hyper Suprime-Cam Survey: the puzzle of HSC~J115252+004733
- Probing Population III Stars in Galaxy IOK-1 at z = 6.96 through He II Emission
- On the dependence between UV luminosity and Lyman-alpha equivalent width in high redshift galaxies
- A Magellan IMACS Spectroscopic Search for Lyman-Alpha Emitting Galaxies at Redshift 5.7
- Star Formation Indicators and Line Equivalent Width in Lyman Alpha Galaxies
- Bayesian Redshift Classification of Emission-line Galaxies with Photometric Equivalent Widths
- Texas Spectroscopic Search for Ly Emission at the End of Reionization I. Constraining the Ly Equivalent Width Distribution at 6.0 < < 7.0
- Empirical Constraints on the Star Formation & Redshift Dependence of the Lyman Alpha `Effective' Escape Fraction
- Stellar Populations of Lyman-alpha Emitters at z=4.86: A Comparison to LBGs
- Ly Emitters with Very Large Ly Equivalent Widths, EW(Ly) Å, at
- The Faint-End Slope of the Redshift 5.7 Lyman Alpha Luminosity Function
- Lyman Alpha and MgII as Probes of Galaxies and their Environments
- The Subaru-XMM-Newton Deep Survey (SXDS) VIII.: Multi-wavelength Identification, Optical/NIR Spectroscopic Properties, and Photometric Redshifts of X-ray Sources
- HST Emission Line Galaxies at z ~ 2: The Ly-alpha Escape Fraction
- Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
- A Plethora of AGN Among Lyman Alpha Galaxies at Low Redshift
- The Ultraluminous Lyman Alpha Luminosity Function at z=6.6
- Non-Gravitational Contributions to the Clustering of Ly-alpha Selected Galaxies: Implications for Cosmological Surveys
- Deep rest-frame far-UV spectroscopy of the giant Lyman-alpha emitter 'Himiko'
- Detections of Faint Lyman-alpha Emitters at z = 5.7: Galaxy Building Blocks and Engines of Reionization
- The impact of Lyman- radiative transfer on large-scale clustering in the Illustris simulation
- Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star forming galaxies at 2<z<3
- Large-scale environment of z~5.7 CIV absorption systems I: projected distribution of galaxies
- A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5<z<6.8: Program Overview and a Sample of the Brightest Lyman-alpha Emitters
- On The Origin of Lyman-alpha Absorption in Nearby Starbursts and Implications for Other Galaxies
- Evaluating Lya Emission as a Tracer of the Largest Cosmic Structure at z~2.47
- The Evolution of the Ultraluminous Ly-alpha Luminosity Function over z=5.7-6.6
- Clustering of Lyman-alpha Emitters Around Quasars at
- RELICS: Strong Lensing analysis of the galaxy clusters Abell S295, Abell 697, MACS J0025.4-1222, and MACS J0159.8-0849
- Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
- Probing high-redshift galaxies with Ly intensity mapping
- Constraining the Lyman Alpha Escape Fraction with Far-Infrared Observations of Lyman Alpha Emitters
- First HETDEX Spectroscopic Determinations of Ly and UV Luminosity Functions at : Bridging a Gap Between Faint AGN and Bright Galaxies
- Galactic winds and stellar populations in Lyman emitting galaxies at z ~ 3.1
- Large-scale environment of CIV absorption systems -II. Spectroscopy of Lyman- emitters
- Lyman-alpha Emitters in Cosmological Simulations I: Lyman-alpha Escape Fraction and Statistical Properties at z=3.1
- Observable Signatures of the low-z Circum-Galactic and Inter-Galactic Medium : UV Line Emission in Simulations
- Planetary Nebulae in Face-On Spiral Galaxies. II. Planetary Nebula Spectroscopy
- Two Lensed Lyman-alpha Emitting Galaxies at z~5
- The Lyman alpha Reference Sample VI: Lyman alpha escape from the edge-on disk galaxy Mrk1486
- A 52 hours VLT/FORS2 spectrum of a bright z~7 HUDF galaxy: no Ly-alpha emission
- The Magellan M2FS Spectroscopic Survey of High-Redshift Galaxies: A Sample of 260 Ly Emitters at Redshift
- Probing the first galaxies with the SKA
- PACS-Herschel FIR detections of Lyman-alpha emitters at 2.0<z<3.5
- COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
- The cross-power spectrum between 21cm emission and galaxies in hierarchical galaxy formation models
- The BOSS Emission-Line Lens Survey V. Morphology and Substructure of Lensed Lyman- Emitters at redshift in the BELLS GALLERY
- Nature and chemical abundances of a sample of Lyman- emitter objects at high redshift
- A Deep Ly Survey in ECDF-S and COSMOS: I. General Properties of Lyman-alpha Emitters at
- Classification and environmental properties of X-ray selected point-like sources in the XMM-LSS field
- SILVERRUSH X: Machine Learning-Aided Selection of LAEs at , , , , , and from the HSC SSP and CHORUS Survey Data
- Continuum Emission by Cooling Clouds
- A Physical Model of Lyman Alpha Emitters
- The impact of the Star Formation Histories on the SFR-M relation at z2
- Acceleration of Galactic Supershells by Lyman Alpha Radiation
- Spectral Energy Distributions of Companion Galaxies to z6 Quasars
- Predicting Lyman-alpha escape fractions with a simple observable: Lyman-alpha in emission as an empirically calibrated star formation rate indicator
- Small-scale Intensity Mapping: Extended Halos as a Probe of the Ionizing Escape Fraction and Faint Galaxy Populations during Reionization
- Ly-alpha emitters: blue dwarfs or supermassive ULIRGs? Evidence for a transition with redshift
- Effects of Star Formation Stochasticity on the Ly-alpha & Lyman Continuum Emission from Dwarf Galaxies during Reionization
- What do observations of the Lyman-alpha fraction tell us about reionization?
- Lyman-α Emitters in the context of hierarchical galaxy formation: predictions for VLT/MUSE surveys
- Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
- Ly alpha emissters at z=6.5 in the SSA22 field: An area more neutral or void at the end of the reionization epoch
- Deep submillimeter and radio observations in the SSA22 field. I. Powering sources and Lyα escape fraction of Lyα blobs
- Rest-frame UV Properties of Luminous Strong Gravitationally Lensed Ly Emitters from the BELLS GALLERY Survey
- Lyα emitters in a cosmological volume I: the impact of radiative transfer
- The discovery of the most UV-Lya luminous star-forming galaxy: a young, dust- and metal-poor starburst with QSO-like luminosities
- CLEAR: Boosted Ly Transmission of the Intergalactic Medium in UV bright Galaxies
- Understanding the redshift evolution of the luminosity functions of Lyman-alpha emitters
- SILVERRUSH. IX. Lya Intensity Mapping with Star-Forming Galaxies at z=5.7 and 6.6: A Possible Detection of Extended Lya Emission at 100 comoving kpc around and beyond the Virial-Radius Scale of Galaxy Dark Matter Halos
- First Systematic Search for Oxygen-Line Blobs at High Redshift: Uncovering AGN Feedback and Star-Formation Quenching
- Cold accretion in early galaxy formation and its Lyman-alpha signatures
- Search for z~7 Ly-alpha emitters with Suprime-Cam at the Subaru Telescope
- Morphological Properties of Lyman Alpha Emitters at Redshift 4.86 in the COSMOS Field: Clumpy Star Formation or Merger?
- The X-ray and radio activity of typical and luminous Lya emitters from z~2 to z~6: evidence for a diverse, evolving population
- The UV-continuum properties of Ly alpha selected galaxies at z=6.5
- [OIII] emitters in the field of the MRC 0316-257 protocluster
- The Obscured Fraction of Quasars at Cosmic Noon
- X-ray Constraints on the Lyman-Alpha Escape Fraction
- Radiative Transfer in Lyα Nebulae: I. Modeling a Continuous or Clumpy Spherical Halo with a Central Source
- Clustering of Ly-alpha emitters around luminous quasars at z = 2-3: an alternative probe of reionization on galaxy formation
- CHORUS. III. Photometric and Spectroscopic Properties of Ly Blobs at
- Search for z~6.96 Ly-alpha emitters with Magellan/IMACS in the COSMOS field
- Faint Resonantly Scattered Lyman Alpha Emission from the Absorption Troughs of Damped Lyman Alpha Systems at z ~ 3
- What Powers Lyman alpha Blobs?
- SHARDS: A global view of the star formation activity at z~0.84 and z~1.23
- Effects of Lyman alpha scattering in the IGM on clustering statistics of Lyman alpha emitters
- Systematic Survey for [OII], [OIII], and H Blobs at : The Implication for Evolution of Galactic-Scale Outflow
- Discovery of a Very Bright and Intrinsically Very Luminous, Strongly Lensed Lyα Emitting Galaxy at z = 2.82 in the BOSS Emission-Line Lens Survey
- CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview
- Eclipsing damped Ly systems in the Sloan Digital Sky Survey Data Release 12
- Measuring the average molecular gas content of star-forming galaxies at
- A deg blind survey for CII], CIII] and CIV at . I: nature, morphologies and equivalent widths
- The environments of Ly blobs I: Wide-field Ly imaging of TN J1338-1942, a powerful radio galaxy at associated with a giant Ly nebula
- Median Surface Brightness Profiles of Lyman- Haloes in the MUSE Extremely Deep Field
- The THESAN project: Lyman-alpha emitter luminosity function calibration
- Constraining C iii] Emission in a Sample of Five Luminous z = 5.7 Galaxies
- X-ray properties of the z ~ 4.5 Lyman-alpha Emitters in the Chandra Deep Field South Region
- The Ly emission from high- galaxies hosting strong Damped Ly systems
- Probing the faint end Luminosity Function of Lyman Alpha Emitters at 3<z<7 behind 17 MUSE lensing clusters
- Cosmology before noon with multiple galaxy populations
- ODIN: Improved Narrowband Ly Emitter Selection Techniques for = 2.4, 3.1, and 4.5
- Finding bright Lyman- emitters with lensing: prospects for Euclid
- Diffuse Lyman-alpha Halos around ~300 Spectroscopically Confirmed Lyman-alpha Emitters at z ~ 5.7
- The Lyman Alpha Reference Sample XI: Efficient Turbulence Driven Lyα Escape and the Analysis of IR, CO and [C II]158 μm
- Discovery of Massive, Mostly Star-formation Quenched Galaxies with Extremely Large Lyman-alpha Equivalent Widths at z ~ 3
- SHARDS Frontier Fields: Physical properties of a low mass Lyman-alpha emitter at z=5.75
- Probing the Metal Enrichment of the Intergalactic Medium at Using the Hubble Space Telescope
- Correlations between H Equivalent Width and Galaxy Properties at : Physical or Selection-driven?
- The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6
- FIR measurements of Ly- emitters at z1.0: dust attenuation from PACS-\emph{Herschel}
- Physical properties of Lyman-alpha emitters at from UV-to-FIR measurements
- Lyman-alpha emitters as tracers of the transitioning Universe
- Observational challenges in Ly-alpha intensity mapping
- GTC Observations of an Overdense Region of LAEs at z=6.5
- Discovery of a giant and luminous Lya+CIV+HeII nebula at z=3.326 with extreme emission line ratios
- Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?
- Differential attenuation in star-forming galaxies at 0.3 1.5 in the SHARDS/CANDELS field
- Design for the First Narrowband Filter for the Dark Energy Camera: Optimizing the LAGER Survey for z ~ 7 Galaxies
- Stellar feedback in a clumpy galaxy at 3.4
- A Search for z=7.3 Lyα Emitters behind Gravitationally Lensing Clusters
- High redshift Lya emitters: clues on the Milky Way infancy
- Galaxies of the Universe. I. Grism-Selected Rest-Frame Optical Emission Line Galaxies
- Probing the Diffuse Lyman-alpha Emission on Cosmological Scales: Lyα Emission Intensity Mapping Using the Complete SDSS-IV eBOSS Survey
- A Spectroscopic Survey of Ly Emitters at over 1.2 Deg
- The impact of gas bulk rotation on the lyman-alpha line
- Variation in the stellar initial mass function from the chromospheric activity of M dwarfs in early-type galaxies
- Revealing the Nature of a Lyman- Halo in a Strongly Lensed Interacting System at
- A deg blind survey for CII], CIII] and CIV at . II: luminosity functions and cosmic average line ratios
- Identifying Lyman Alpha Emitters powered by AGNs
- Determining the systemic redshift of Lyman-alpha emitters with neural networks and improving the measured large-scale clustering
- Emission Line Galaxies in the SHARDS Frontier Fields I: Candidate Selection and the Discovery of Bursty Hα Emitters
- Spatially-resolved Spectroscopic Analysis of Ly Haloes: Radial Evolution of the Ly Line Profile out to 60 kpc
- Molecular hydrogen in Lyman Alpha Emitters
- Evolution of Star Formation in the UKIDSS Ultra Deep Survey Field - II. Star Formation as a Function of Stellar Mass Between z=1.46 and z=0.63
- Linking UV spectral properties of MUSE Ly-alpha emitters at z>3 to Lyman continuum escape
- The Utility of Lyman-alpha Emission Lines as a Probe of Interactions between High Redshift Galaxies and their Environments
- Constraining Reionization with Lyman Alpha Emitting Galaxies
- Void Probability Function of Simulated Surveys of high-redshift Lyman-Alpha Emitters
- Empowering line intensity mapping to study early galaxies
- Lyman Alpha line properties at and their environmental dependence: a case study around a massive proto-cluster
- The OTELO survey: Faint end of the luminosity function of [OII] emitters at <z>= 1.43
- Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
- Galaxy populations in protoclusters at cosmic noon
- LOFAR properties of SILVERRUSH Ly emitter candidates in the ELAIS-N1 field
- Probing the Long Gamma-Ray Burst Progenitor by Lyman-alpha Emission of Host Galaxies
- Extinction Correction Significantly Influences the Estimate of Ly Escape Fraction
- Subaru FOCAS survey of z=7-7.1 Lyα emitters: a test for z >~ 7 Lyα photometric luminosity functions
- Observations of Ly Emitters at High Redshift
- Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
- On the star formation efficiency in high redshift Lyman-α emitters
- Photometric IGM Tomography: Efficiently Mapping Quasar Light Echoes with Deep Narrow Band Imaging
- Filter Induced Bias in Lyα Emitter Surveys: A Comparison Between Standard and Tunable Filters. Gran Telescopio Canarias Preliminary Results
- Lyman break and UV-selected galaxies at I. Stellar populations from ALHAMBRA survey
- Effects of photon trapping on the Lyman-alpha properties of star-forming galaxies
- Is the Bremer Deep Field ionised, at z~7?
- The miniJPAS & J-NEP surveys: Identification and characterization of the Ly Emitter population and the Ly Luminosity Function
- A z ~ 5.7 Lyα Emission Line with an Ultra Broad Red Wing
- Probing the cosmic web in Ly emission over large scales: an Intensity Mapping forecast for DECaLS/BASS and DESI
- Lyman- emission from a WISE-selected optically faint powerful radio galaxy M151304.72-252439.7 at = 3.132
- Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly emitters and IGM transmission in the COSMOS field at
- A search for Ly-alpha emitters around a concentrated-region of strong Ly-alpha absorbers at z=2.3
- New Results from the Magellan IMACS Spectroscopic Lyman Alpha Survey: NICMOS Observations of Lyman Alpha emitters at z=5.7
- SEURAT: SPH scheme extended with ultraviolet line radiative transfer
- The Intrinsic Distribution of Lyman- Halos
- The PAU Survey: The quasar UV and Ly luminosity functions at
- The importance of nebular emission for SED modeling of distant star-forming galaxies
- Three-Dimensional Stacking as a Line Intensity Mapping Statistic
- Deep Hubble Space Telescope Imaging on the Extended Ly Emission of a QSO at with Damped Lyman Alpha System as a Natural Coronagraph
- The contribution of faint Lyman- emitters to extended Lyman- halos constrained by MUSE clustering measurements
- 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
- Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at
- MUSUBI (MegaCam Ultra-deep Survey: -Band Imaging)-Data for the COSMOS and SXDS Fields
- Understanding Lyman-alpha emitters
- LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at
- Lyman- Emitting Galaxies (LAEs) at Cosmic Dawn: Implications and Predictions
- Near-IR narrow-band imaging with CIRCE at the Gran Telescopio Canarias: Searching for Ly-emitters at
- Modelling the Evolution of Ly Blobs and Ly Emitters
- The search for Population III stars
- Quantifying the effect of field variance on the H luminosity function with the New Numerical Galaxy Catalogue (GC)
- Evolutionary synthesis models as a tool and guide towards the first galaxies
- Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman- Emitters
- Searching for Pop III stars and galaxies at high redshift
- The effect of ionizing background fluctuations on the spatial correlations of high redshift Ly-emitting galaxies
- Joint Lyα emitters - quasars reionization constraints
- Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-Power Spectrum
- HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy
- The MUSE Hubble Ultra Deep Field Survey XIV. The evolution of the Lya emitter fraction from z=3 to z=6
- X-ray luminosity functions of different morphological and X-ray type AGN populations
- Can luminous Lyman alpha emitters at 5.7 and 6.6 suppress star formation?
- Luminosities, Masses and Star Formation Rates of Galaxies at High Redshift (IAU279 conference proceedings)
- Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
- Clustering analysis of medium-band selected high-redshift galaxies
- The HiZELS/UKIRT large area survey for bright Lyman-alpha emitters at z~9