A Steep Faint-End Slope of the UV Luminosity Function at z~2-3: Implications for the Global Stellar Mass Density and Star Formation in Low Mass Halos

Abstract

We use the deep ground-based optical photometry of the Lyman Break Galaxy (LBG) Survey to derive robust measurements of the faint-end slope (alpha) of the UV LF at redshifts 1.9<z<3.4. Our sample includes >2000 spectroscopic redshifts and ~31000 LBGs in 31 spatially-independent fields over a total area of 3261 arcmin^2. These data allow us to select galaxies to 0.07L* and 0.10L* at z~2 and z~3, respectively. A maximum likelihood analysis indicates steep values of alpha(z=2)=-1.73+/-0.07 and alpha(z=3)=-1.73+/-0.13. This result is robust to luminosity dependent systematics in the Ly-alpha equivalent width and reddening distributions, is similar to the steep values advocated at z>4, and implies that ~93% of the unobscured UV luminosity density at z~2-3 arises from sub-L* galaxies. With a realistic luminosity dependent reddening distribution, faint to moderately luminous galaxies account for >70% and >25% of the bolometric luminosity density and present-day stellar mass density, respectively, when integrated over 1.9<z<3.4. We find a factor of 8-9 increase in the star formation rate density between z~6 and z~2, due to both a brightening of L* and an increasing dust correction proceeding to lower redshifts. The previously observed discrepancy between the integral of the star formation history and stellar mass density measurements at z~2 may be reconciled by invoking a luminosity dependent reddening correction to the star formation history combined with an accounting for the stellar mass contributed by UV-faint galaxies. The steep and relatively constant alpha of the UV LF at z>2 contrasts with the shallower value inferred locally, suggesting that the evolution in the faint-end slope may be dictated simply by the availability of low mass halos capable of supporting star formation at z<2. [Abridged]

29 pages, 15 figures, 7 tables; accepted for publication in ApJ

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• The Stacked Lyman-Alpha Emission Profile from the Circum-Galactic Medium of z~2 Quasars
• The Universe at extreme magnification
• An Empirical Study of the Relationship between Lyα and UV selected Galaxies: Do Theorists and Observers `Select' the Same Objects?
• An extreme blue nugget, UV-bright starburst at z=3.613 with ninety per cent of Lyman continuum photon escape
• The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey
• The Very Faint End of the UV Luminosity Function over Cosmic Time: Constraints from the Local Group Fossil Record
• An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
• Star formation history, dust attenuation and extragalactic background light
• On the Evolution of the Cosmic Ionizing Background
• Star Formation in Luminous Quasars at 2<z<3
• The history of star formation from the cosmic infrared background anisotropies
• Environmentally Driven Global Evolution of Galaxies
• Young Galaxy Candidates in the Hubble Frontier Fields - III. MACSJ0717.5+3745
• Ultraviolet Luminosity Density of the Universe During the Epoch of Reionization
• Star Formation from DLA Gas in the Outskirts of Lyman Break Galaxies at z~3
• The LBT Bootes Field Survey: I. The Rest-frame UV and Luminosity Functions and Clustering of Bright Lyman Break Galaxies at z~3
• Revealing Type Ia supernova physics with cosmic rates and nuclear gamma rays
• The UV-brightest Lyman continuum emitting star-forming galaxy
• A Dual Narrowband Survey for Hα Emitters at z=2.2: Demonstration of the Technique and Constraints on the Hα Luminosity Function
• The Swift Gamma-Ray Burst redshift distribution: selection biases and optical brightness evolution at high-z?
• The SCUBA-2 Cosmology Legacy Survey: the submillimetre properties of Lyman break galaxies at z=3-5
• Supernova Relic Neutrinos and the Supernova Rate Problem: Analysis of Uncertainties and Detectability of ONeMg and Failed Supernovae
• Dwarf Galaxy Formation with H2-Regulated Star Formation: II. Gas-Rich Dark Galaxies at Redshift 2.5
• Local Analogs for High-redshift Galaxies: Resembling the Physical Conditions of the Interstellar Medium in High-redshift Galaxies
• The Quest for Dusty Star-forming Galaxies at High Redshift z>4
• Demonstrating the Feasibility of Line Intensity Mapping Using Mock Data of Galaxy Clustering from Simulations
• Resolving the Galaxies within a Giant Lya Nebula: Witnessing the Formation of a Galaxy Group?
• Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies
• Intensity mapping of H-alpha, H-beta, [OII] and [OIII] lines at z<5
• UV & U-band luminosity functions from CLAUDS and HSC-SSP -- I. Using four million galaxies to simultaneously constrain the very faint and bright regimes to $z\sim 3$
• Intermediate-Mass Black Hole Growth and Feedback in Dwarf Galaxies at High Redshifts
• Stellar Populations of Highly Magnified Lensed Galaxies: Young Starbursts at z~2
• Optimized Photometric Redshifts for the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS)
• O VI Emission Imaging of a Galaxy with the Hubble Space Telescope: a Warm Gas Halo Surrounding the Intense Starburst SDSS J115630.63+500822.1
• Properties of QSO Metal Line Absorption Systems at High Redshifts: Nature and Evolution of the Absorbers and New Evidence on Escape of Ionizing Radiation from Galaxies
• A direct calibration of the IRX-β relation in Lyman-break Galaxies at z=3-5
• Galactic Winds in Cosmological Simulations of the Circumgalactic Medium
• Effect of radiative transfer on damped Lyman-alpha and Lyman limit systems in cosmological SPH simulations
• UVUDF: UV Luminosity Functions at the cosmic high-noon
• Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field
• Galaxy evolution in protoclusters
• Discovery of Lyman Break Galaxies at z~7 from the ZFOURGE Survey
• The UV colours and dust attenuation of Lyman-break galaxies
• Pair-Instability Supernovae via Collision Runaway in Young Dense Star Clusters
• Detection of hot, metal-enriched outflowing gas around $z\approx$2.3 star-forming galaxies in the Keck Baryonic Structure Survey
• Stars, Dust, and the Growth of UV-Selected Sub-L* Galaxies at Redshift z~2
• Star formation and dust extinction properties of local galaxies from AKARI-GALEX All-Sky Surveys: First results from most secure multiband sample from FUV to FIR
• Spatially Resolved Emission of a High Redshift DLA Galaxy with the Keck/OSIRIS IFU
• Winds of change: reionization by starburst galaxies
• The Evolution of the Rest-frame V-band Luminosity Function from z=4: A Constant Faint-end Slope over the Last 12 Gyr of Cosmic History
• Cosmological Implications of a Stellar Initial Mass Function that Varies with the Jeans Mass in Galaxies
• Nature of Lyman Alpha Blobs: Powered by Extreme Starbursts
• A Study of Massive and Evolved Galaxies at High Redshift
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population
• The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4
• How Do Galaxies trace a large scale structure?: A case study around a massive protocluster at $z=3.13$
• The Ionizing Photon Production Efficiency (${\xi }_{ion}$) Of Lensed Dwarf Galaxies At $z\sim 2$
• A spectroscopic measurement of galaxy formation timescales with ROLES
• The VIMOS Ultra-Deep Survey: A major merger origin for the high fraction of galaxies at $2<z<6$ with two bright clump
• The Unchanging Circumgalactic Medium Over the Past 11 Billion Years
• Infrared Spectra and Spectral Energy Distributions for Dusty Starbursts and AGN
• On Lya emission in z~3-6 UV-selected galaxies
• A joint model for the emission and absorption properties of damped Lyman alpha absorption systems
• The KBSS-KCWI Survey: The connection between extended Ly$\alpha$ halos and galaxy azimuthal angle at $z\sim 2-3$
• Observing the first galaxies
• Studying reionization with the next generation of Ly-alpha emitter surveys
• The HDUV Survey: Six Lyman Continuum Emitter Candidates at z~2 Revealed by HST UV Imaging
• A High Space Density of Luminous Lyman Alpha Emitters at z~6.5
• The [OIII]$\lambda 5007$ equivalent width distribution at z $\sim 2$: The redshift evolution of the extreme emission line galaxies
• Measures of star formation rates from Infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields
• Origin of Cosmic Chemical Abundances
• A bright, spatially extended lensed galaxy at z = 1.7 behind the cluster RCS2 032727-132623
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• Stellar Populations of Lyman Break Galaxies at z=1-3 in the HST/WFC3 Early Release Science Observations
• Diversity of Galaxy Dust Attenuation Curves Drives the Scatter in the IRX-beta Relation
• Detection of three Gamma-Ray Burst host galaxies at $z\sim 6$
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies
• Directly imaging damped Lyman-alpha galaxies at z>2. I: Methodology and First Results
• The Impact of Strong Gravitational Lensing on Observed Lyman-Break Galaxy Numbers at 4<z<8 in the GOODS and the XDF Blank Fields
• Deep Keck u-band imaging of the Hubble Ultra Deep Field: A catalog of z~3 Lyman Break Galaxies
• Infrared Classification and Luminosities For Dusty AGN and the Most Luminous Quasars
• Illuminating the Darkest Gamma-Ray Bursts with Radio Observations
• A Method for Measuring the Bias of High-Redshift Galaxies from Cosmic Variance
• The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at $7<z<8$
• The cosmic abundance of cold gas in the local Universe
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts $z$$\simeq$2.3-4.1
• The evolution of the star formation rate function and cosmic star formation rate density of galaxies at $z\sim 1-4$
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
• A Ks and IRAC Selection of High-Redshift Extremely Red Objects
• Discovery of the optical afterglow and host galaxy of short GRB181123B at $z=1.754$: Implications for Delay Time Distributions
• The Star Formation Rate Efficiency of Neutral Atomic-dominated Hydrogen Gas in the Outskirts of Star Forming Galaxies from z~1 to z~3
• An Hα view of galaxy build-up in the first 2 Gyr: luminosity functions at z~4-6.5 from NIRCam/grism spectroscopy
• The Circumgalactic Medium of Extreme Emission Line Galaxies at z ~ 2: Resolved Spectroscopy and Radiative Transfer Modeling of Spatially Extended Lyman-alpha Emission in the KBSS-KCWI Survey
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• A large, deep 3 deg${}^2$ survey of H$\alpha$, [OIII], and [OII] emitters from LAGER: constraining luminosity functions
• Lyman-alpha Emitters in Cosmological Simulations I: Lyman-alpha Escape Fraction and Statistical Properties at z=3.1
• A census of galaxy constituents in a Coma Progenitor observed at z>3
• HerMES: Herschel-SPIRE observations of Lyman Break Galaxies
• The UV Continuum of z > 1 Star-forming Galaxies in the Hubble Ultraviolet UltraDeep Field
• CASSOWARY 20: a Wide Separation Einstein Cross Identified with the X-shooter Spectrograph
• The nature of damped HI absorbers probed by cosmological simulations: satellite accretion and outflows
• Simulating the infrared sky with a Spritz
• Lyman-Break Galaxies at $z\sim 3$ in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission
• Dust properties of Lyman break galaxies in cosmological simulations
• A Deep Ly$\alpha$ Survey in ECDF-S and COSMOS: I. General Properties of Lyman-alpha Emitters at $z\sim 2$
• The Properties of Hα Emission-Line Galaxies at z = 2.24
• Revisiting the Cosmic Star Formation History: Caution on the Uncertainties in Dust Correction and Star Formation Rate Conversion
• The Redshift One LDSS-3 Emission line Survey (ROLES) II: Survey method and z~1 mass-dependent star-formation rate density
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• Probing High-Redshift Galaxy Formation at the Highest Luminosities: New Insights from DEIMOS Spectroscopy
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• Tracing the Mass Growth and Star Formation Rate Evolution of Massive Galaxies from z~6 to z~1 in the Hubble Ultra-Deep Field
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• The discovery of the most UV-Lya luminous star-forming galaxy: a young, dust- and metal-poor starburst with QSO-like luminosities
• Understanding the redshift evolution of the luminosity functions of Lyman-alpha emitters
• Rest-frame UV Properties of Luminous Strong Gravitationally Lensed Ly$\alpha$ Emitters from the BELLS GALLERY Survey
• Constraints on the Redshift Evolution of the L_X-SFR Relation from the Cosmic X-Ray Backgrounds
• A New Constraint on the Physical Nature of Damped Lyman Alpha Systems
• The UDF05 Follow-up of the Hubble Ultra Deep Field. III. The Luminosity Function at z~6
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.6 from HSC-SSP PDR2 and CHORUS
• Evolution of Galaxy Luminosity Function Using Photometric Redshifts
• On the inconsistency between the estimates of cosmic star formation rate and stellar mass density of high redshift galaxies
• Dust attenuation of the nebular regions and optical emission lines of $z\sim 2$ star-forming galaxies
• The unseen host galaxy and high dispersion measure of a precisely-localised Fast Radio Burst suggests a high-redshift origin
• 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
• An Updated Ultraviolet Catalog of GALEX Nearby Galaxies
• Constraining the epoch of reionization from the observed properties of the high-z Universe
• Gamma-ray Bursts and the Early Star-formation History
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Universe opacity and CMB
• Optical dropout galaxies lensed by the cluster A2667
• Probing the Star Formation Main Sequence down to $10^8$ M${}_{\odot }$ at $1.0<z<3.0$
• Broadband Imaging Segregation of z ~ 3 Ly-alpha Emitting and Ly-alpha Absorbing Galaxies
• Star Formation Rates and Stellar Masses of H-alpha Selected Star-Forming Galaxies at z=0.84: A Quantification of the Downsizing
• Imaging of diffuse HI absorption structure in the SSA22 proto-cluster region at z = 3.1
• Molecular gas properties of UV-luminous star-forming galaxies at low redshift
• Cosmic star formation rate: a theoretical approach
• The Ly$\alpha$ emission from high-$z$ galaxies hosting strong Damped Ly$\alpha$ systems
• An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies
• Origin Of The High Energy Cosmic Neutrino Background
• The Flatness and Sudden Evolution of the Intergalactic Ionizing Background
• Dust Attenuation in Clumpy, Star-Forming Galaxies at 0.07 < z < 0.14
• HiZELS: the High Redshift Emission Line Survey with UKIRT
• The bright-end of the luminosity function at z~9
• Discovery of an unusually compact lensed Lyman Break Galaxy from the Hyper Suprime-Cam Survey
• The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6
• Spectroscopy of CASSOWARY gravitationally-lensed galaxies in SDSS: characterisation of an extremely bright reionization-era analog at $z=1.42$
• Abundant Serendipitous Emission Line Sources with JWST/NIRSpec
• The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmology
• Galaxy formation with cold gas accretion and evolving stellar initial mass function
• Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function
• Subaru narrow-band imaging search for Lyman continuum from galaxies at z>3 in the GOODS-N field
• Far-Infrared Properties of Lyman Break Galaxies from Cosmological Simulations
• The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas
• High-Redshift Galaxy Surveys and the Reionization of the Universe
• The Redshift Distribution of Intervening Weak MgII Quasar Absorbers and a Curious Dependence on Quasar Luminosity
• Metal Abundances of KISS Galaxies. V. Nebular Abundances of Fifteen Intermediate Luminosity Star-Forming Galaxies
• The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.6 and 1.2
• Star formation in high redshift galaxies including Supernova feedback: effect on stellar mass and luminosity functions
• High redshift LBGs from deep broadband imaging for future spectroscopic surveys
• A${}^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4<z<5$
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• Probing the Diffuse Lyman-alpha Emission on Cosmological Scales: Lyα Emission Intensity Mapping Using the Complete SDSS-IV eBOSS Survey
• Narrow C IV absorption doublets on quasar spectra of the Baryon Oscillation Spectroscopic Survey
• A UV Ultra-luminous Lyman Break Galaxy at Z=2.78 in NDWFS Bootes Field
• RCS2 J232727.6-020437: An Efficient Cosmic Telescope at $z=0.6986$
• Universe opacity and EBL
• Near-identical star formation rate densities from H$\alpha$ and FUV at redshift zero
• The star-forming main sequence and the contribution of dust-obscured star formation since $z\sim 4$ from the FUV+IR luminosity functions
• Spritz is sparkling: simulated CO and [CII] luminosities
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
• Long Gamma Ray Bursts Trace The Star Formation History
• Missing dust signature in the cosmic microwave background
• Stability and Ly$\alpha$ emission of Cold Stream in the Circumgalactic Medium: impact of magnetic fields and thermal conduction
• Galaxy populations in protoclusters at cosmic noon
• Science Case and Requirements for the MOSAIC Concept for a Multi-Object Spectrograph for the European Extremely Large Telescope
• The OTELO survey: Faint end of the luminosity function of [OII] emitters at <z>= 1.43
• Lyman Alpha line properties at $z\simeq 3.78$ and their environmental dependence: a case study around a massive proto-cluster
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• High-$z$ Universe probed via Lensing by QSOs (HULQ) I. Number Estimates of QSO-QSO and QSO-Galaxy Lenses
• Bayesian Multi-line Intensity Mapping
• UV slope of z$\sim$3 bright ($L>L^{\ast }$) Lyman-break galaxies in the COSMOS field
• On the star formation efficiency in high redshift Lyman-α emitters
• SED-inferred properties and morphology of Lyman-break galaxies at $z\sim 1$ in the CDF-S
• Seeking the Epoch of Maximum Luminosity for Dusty Quasars
• A physical model for the redshift evolution of high-z Lyman-Break Galaxies
• 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
• Fast Extragalactic X-ray Transients From Binary Neutron Star Mergers
• Probing Patchy Reionization with the Void Probability Function of Lyman-$\alpha$ Emitters
• Comparing Ultraviolet and Infrared-Selected Starburst Galaxies in Dust Obscuration and Luminosity
• MUSUBI (MegaCam Ultra-deep Survey: $u^{\ast }$-Band Imaging)-Data for the COSMOS and SXDS Fields
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• Lyman-alpha at Cosmic Noon I: Ly-alpha Spectral Type Selection of z ~ 2-3 Lyman Break Galaxies with Broadband Imaging
• KBSS-InCLOSE I: Design and First Results from the Inner CGM of QSO Line Of Sight Emitting Galaxies at z~2-3
• Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at $z\sim 2.1-3.6$
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• An optically-dark merging system at z~6 detected by JWST
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• Considering light-matter interactions in the Friedmann equations
• SDSS J1059+4251, a highly magnified z ~ 2.8 star-forming galaxy: ESI observations of the rest-frame UV spectrum
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• The Cosmic Evolution of CIV Absorbers at $1.4<z<4.5$: Insights from $100,000$ Systems in DESI Quasars
• From Gas to Stars over Cosmic Time
• Dust contribution to the panchromatic galaxy emission
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Constraining $z\lesssim 2$ ultraviolet emission with the upcoming ULTRASAT satellite
• Quenching Global Star Formation: Dominance of Gravitational Shock Heating at z<2
• CECILIA: Ultra-Deep Rest-Optical Spectra of Faint Galaxies at Cosmic Noon
• Lyman-alpha at Cosmic Noon II: The relationship between kinematics and Lyman-alpha in z~2-3 Lyman Break Galaxies
• High redshift galaxies in the ALHAMBRA survey: II. strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z <= 4.5 by PDF analysis
• Luminosities, Masses and Star Formation Rates of Galaxies at High Redshift (IAU279 conference proceedings)
• The build-up of mass in UV-selected sub-L* galaxies at z~2
• Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6
• The 5 Gyr evolution of sub-M* galaxies
• Extended H$\alpha$ over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at $z\sim 2$