The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies

Abstract

We use a newly assembled large sample of 3,545 star-forming galaxies with secure spectroscopic, grism, and photometric redshifts at z=1.5-2.5 to constrain the relationship between UV slope (beta) and dust attenuation (L(IR)/L(UV)=IRX). Our sample benefits from the combination of deep Hubble WFC3/UVIS photometry from the Hubble Deep UV (HDUV) Legacy survey and existing photometric data compiled in the 3D-HST survey, and extends the range of UV luminosity and beta probed in previous UV-selected samples. IRX is measured using stacks of deep Herschel/PACS 100 and 160 micron data, and the results are compared with predictions of the IRX-beta relation for different assumptions of the stellar population model and obscuration curve. We find that z=1.5-2.5 galaxies have an IRX-beta relation that is consistent with the predictions for an SMC extinction curve if we invoke sub-solar metallicity models that are currently favored for high-redshift galaxies, while the commonly assumed starburst attenuation curve over-predicts the IRX at a given beta by a factor of ~3. The IRX of high-mass (M*>10^9.75 Msun) galaxies is a factor of >4 larger than that of low-mass galaxies, lending support for the use of stellar mass as a proxy for attenuation. The commonly observed trend of fainter galaxies having bluer beta may simply reflect bluer intrinsic UV slopes for such galaxies, rather than lower obscurations. The IRX-beta for young/low-mass galaxies implies a dust curve that is steeper than the SMC, suggesting a lower attenuation at a given beta relative to older/more massive galaxies. The lower attenuations and higher ionizing photon output implied by low metallicity stellar population models point to Lyman continuum production efficiencies, xi_ion, that may be elevated by a factor of ~2 relative to the canonical value for L* galaxies, aiding in their ability to keep the universe ionized at z~2. [Abridged]

arXiv comment22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal

References in corpus (144)

• Stellar population synthesis at the resolution of 2003
• The chemical composition of the Sun
• Galactic Stellar and Substellar Initial Mass Function
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
• Star Formation in the Milky Way and Nearby Galaxies
• CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• EAZY: A Fast, Public Photometric Redshift Code
• Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
• Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
• Metallicity Calibrations and the Mass-Metallicity Relation for Star-Forming Galaxies
• Lyman Break Galaxies at z>4 and the Evolution of the UV Luminosity Density at High Redshift
• A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
• A Redshift Survey of the Submillimeter Galaxy Population
• Dust Absorption And The Ultraviolet Luminosity Density At z \approx 3 As Calibrated By Local Starburst Galaxies
• GOODS-Herschel: an infrared main sequence for star-forming galaxies
• Cool Gas in High Redshift Galaxies
• Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
• Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust Enshrouded Star Formation Rate
• The Mass-Metallicity Relation at z~2
• 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
• AMAZE. I. The evolution of the mass-metallicity relation at z>3
• The Mid-Infrared Spectrum of Star-Forming Galaxies: Global Properties of PAH Emission
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• The Infrared Spectral Energy Distribution of Normal Star-Forming Galaxies: Calibration at Far-Infrared and Submillimeter Wavelengths
• Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones
• Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
• The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
• Dusty Star-Forming Galaxies at High Redshift
• The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies
• Identifying Luminous AGN in Deep Surveys: Revised IRAC Selection Criteria
• Strong Nebular Line Ratios in the Spectra of z~2-3 Star-forming Galaxies: First Results from KBSS-MOSFIRE
• Determining Star Formation Rates for Infrared Galaxies
• UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History
• The Chandra Deep Field-South Survey: 4 Ms Source Catalogs
• The Mass-Metallicity Relation with the Direct Method on Stacked Spectra of SDSS Galaxies
• 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
• Dust Formation in Primordial Type II Supernovae
• New Constraints on Cosmic Reionization from the 2012 Hubble Ultra Deep Field Campaign
• Star Formation and Dust Attenuation Properties in Galaxies from a Statistical UV-to-FIR Analysis
• UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z>=4 star-forming galaxies
• The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang
• Reionization after Planck: The Derived Growth of the Cosmic Ionizing Emissivity now matches the Growth of the Galaxy UV Luminosity Density
• UV Continuum Slope and Dust Obscuration from z~6 to z~2: The Star Formation Rate Density at High Redshift
• The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations
• The Ultraviolet Spectrum of MS 1512-cB58: An Insight into Lyman Break Galaxies
• Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4
• Reconciling the Stellar and Nebular Spectra of High Redshift Galaxies
• Multi-wavelength Observations of Dusty Star Formation at Low and High Redshift
• A dusty, normal galaxy in the epoch of reionization
• A deep ALMA image of the Hubble Ultra Deep Field
• Unusual Broad Absorption Line Quasars from the Sloan Digital Sky Survey
• Stellar Population Effects on the Inferred Photon Density at Reionization
• Dust Obscuration and Metallicity at High Redshift: New Inferences from UV, H-alpha, and 8 Micron Observations of z~2 Star-Forming Galaxies
• Metallicity Effects on Mid-Infrared Colors and the 8 micron PAH Emission in Galaxies
• Infared Observations of Nebular Emission Lines from Galaxies at z = 3
• Spectral synthesis including massive binaries
• Star Formation and Extinction in Redshift z~2 Galaxies: Inferences from Spitzer MIPS Observations
• Dust attenuation in the nearby Universe: comparison between galaxies selected in the ultraviolet or in the infrared
• The infrared luminosity function of galaxies at redshifts z=1 and z~2 in the GOODS fields
• Mapping the Evolution of High Redshift Dusty Galaxies with Submillimeter Observations of a Radio-Selected Sample
• The Characteristic Star Formation Histories of Galaxies at Redshifts z~2-7
• The Hubble Space Telescope Wide Field Camera 3 Early Release Science data: Panchromatic Faint Object Counts for 0.2-2 microns wavelength
• ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass
• Star formation history and dust attenuation in galaxies drawn from ultraviolet surveys
• Spectroscopic detection of CIV in a galaxy at z=7.045: Implications for the ionizing spectra of reionization-era galaxies
• (Star)bursts of FIRE: observational signatures of bursty star formation in galaxies
• Radial distribution of stars, gas and dust in SINGS galaxies. II. Derived dust properties
• A Spectroscopic Survey of Redshift 1.4<z<3.0 Galaxies in the Goods-North Field: Survey Description, Catalogs, and Properties
• GOODS-Herschel Measurements of the Dust Attenuation of Typical Star-Forming Galaxies at High Redshift: Observations of UV-Selected Galaxies at z~2
• The assembly of "normal" galaxies at z=7 probed by ALMA
• Stellar Evolutionary Effects on the Abundances of PAH and SN-Condensed Dust in Galaxies
• Far-Infrared Galaxies in the Far-Ultraviolet
• The Lyman-Continuum Photon Production Efficiency xi_{ion} of z~4-5 Galaxies from IRAC-based Halpha Measurements: Implications for the Escape Fraction and Cosmic Reionization
• Direct measurements of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates
• A Census of Optical and Near-Infrared Selected Star-Forming and Passively Evolving Galaxies at Redshift Z~2
• GOODS-Herschel:dust attenuation properties of UV selected high redshift galaxies
• Star formation in AGN hosts in GOODS-N
• Are Dusty Galaxies Blue? Insights on UV Attenuation from Dust-Selected Galaxies
• Tracing the reionization epoch with ALMA: [CII] emission in z~7 galaxies
• A Model for the Origin of Bursty Star Formation in Galaxies
• FUSE Measurements of Far-Ultraviolet Extinction. III. The Dependence on R(V) and Discrete Feature Limits from 75 Galactic Sightlines
• The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\alpha$ and H$\beta$ emission lines at z ~ 2
• Ultra-faint Ultraviolet Galaxies at z~2 Behind the Lensing Cluster Abell 1689: the Luminosity Function, Dust Extinction and Star Formation Rate Density
• Properties of $z\sim 3-6$ Lyman Break Galaxies. II. Impact of nebular emission at high redshift
• The UV Properties of Star Forming Galaxies I: HST WFC3 Observations of Very-high Redshift Galaxies
• The IRX-beta relation on sub-galactic scales in star-forming galaxies of the Herschel Reference Survey
• Breaking the Curve with CANDELS: A Bayesian Approach to Reveal the Non-Universality of the Dust-Attenuation Law at High Redshift
• A search for the submillimetre counterparts to Lyman break galaxies
• The relationship between star formation rates and mid-infrared emission in galactic disks
• Warm dust and aromatic bands as quantitative probes of star-formation activity
• The effect of stellar evolution uncertainties on the rest-frame ultraviolet stellar lines of CIV and HeII in high-redshift Lyman-break galaxies
• A New Star-Formation Rate Calibration from Polycyclic Aromatic Hydrocarbon Emission Features and Application to High Redshift Galaxies
• The Connection Between Reddening, Gas Covering Fraction, and the Escape of Ionizing Radiation at High Redshift
• HerMES: dust attenuation and star formation activity in UV-selected samples from z~4 to z~1.5
• Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4
• [CII] emission in z ~ 6 strongly lensed, star-forming galaxies
• The Effects of Stellar Rotation. I. Impact on the Ionizing Spectra and Integrated Properties of Stellar Populations
• GMASS ultradeep spectroscopy of galaxies at z ~ 2. IV. The variety of dust populations
• Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties
• The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
• Spectroscopic Measurements of the Far-Ultraviolet Dust Attenuation Curve at z~3
• A Hard Ionizing Spectrum in z=3-4 Ly-alpha Emitters with Intense [OIII] Emission: Analogs of Galaxies in the Reionization Era?
• X-Ray and Radio Emission from UV-Selected Star Forming Galaxies at Redshifts 1.5<Z<3.0 in the GOODS-North Field
• HerMES: Unveiling obscured star formation - the far infrared luminosity function of ultraviolet-selected galaxies at z~1.5
• The problematic growth of dust in high redshift galaxies
• The Bursty Star Formation Histories of Low-mass Galaxies at $0.4<z<1$ Revealed by Star Formation Rates Measured from H$\beta$ and FUV
• Properties of z~3-6 Lyman break galaxies. II. Testing star formation histories and the SFR-mass relation with ALMA and near-IR spectroscopy
• The Evolution Of The Faint End Of The UV Luminosity Function During The Peak Epoch Of Star Formation (1<z<3)
• New constraints on dust emission and UV attenuation of z=6.5-7.5 galaxies from millimeter observations
• GOODS-HERSCHEL: evidence for a UV extinction bump in galaxies at z > 1
• Consequences of bursty star formation on galaxy observables at high redshifts
• Ultraviolet through Infrared Spectral Energy Distributions from 1000 SDSS Galaxies: Dust Attenuation
• UV-dropout Galaxies in the GOODS-South Field from WFC3 Early Release Science Observations
• Dust properties of Lyman break galaxies at $z\sim 3$
• Spitzer Observations of the z=2.73 Lensed Lyman Break Galaxy, MS1512-cB58
• The First Billion Years project: constraining the dust attenuation law of star-forming galaxies at z $\simeq$ 5
• A Multi-wavelength View of the Star Formation Activity at z~3
• ISOCAM view of the starburst galaxies M82, NGC253, and NGC1808
• Interpreting the observed UV continuum slopes of high-redshift galaxies
• Polycyclic Aromatic Hydrocarbon and Emission Line Ratios in Active Galactic Nuclei and Starburst Galaxies
• The Dust Attenuation of Star-forming Galaxies at $z\sim 3$ and Beyond: New Insights from ALMA Observations
• Formation History of Polycyclic Aromatic Hydrocarbons in Galaxies
• Obscured star formation in the central region of the dwarf galaxy NGC5253
• Anomalously low PAH emission from low-luminosity galaxies
• Dust emission from the lensed Lyman break galaxy cB58
• The MOSDEF Survey: Metallicity Dependence of the PAH Emission at High Redshift and Implications for 24 micron-inferred IR Luminosities and Star Formation Rates at z~2
• A Dual Narrowband Survey for Hα Emitters at z=2.2: Demonstration of the Technique and Constraints on the Hα Luminosity Function
• Molecular gas properties of a lensed star-forming galaxy at z~3.6: a case study
• Mid- to far infrared properties of star-forming galaxies and active galactic nuclei
• Extinction curve template for intrinsically reddened quasars
• Star formation histories, extinction, and dust properties of strongly lensed z~1.5-3 star-forming galaxies from the Herschel Lensing Survey
• Evidence for a wide range of UV obscuration in z ~ 2 dusty galaxies from the GOODS-Herschel survey
• The infrared emission of ultraviolet selected galaxies from z = 0 to z=1
• The ultraviolet properties of Luminous Infrared Galaxies at z ~ 0.7: is there any evolution in their dust attenuation?
• The Dust Attenuation Curve versus Stellar Mass for Emission Line Galaxies at z ~ 2
• The Starburst Nature of Lyman-Break Galaxies: Testing UV Extinction with X-rays
• FUSE Measurements of Far Ultraviolet Extinction. I. Galactic Sight Lines
• The Nature of the Second Parameter in the IRX-beta Relation for Local Galaxies
• UV to IR Luminosities and Dust Attenuation Determined from ~4000 K-Selected Galaxies at 1<z<3 in the ZFOURGE Survey
• A resolved map of the infrared excess in a Lyman Break Galaxy at z=3
• Dust attenuation of the nebular regions and optical emission lines of $z\sim 2$ star-forming galaxies
• Deep 15um AKARI observations in the CDFS: estimating dust luminosities for a MIR-selected sample and for Lyman Break Galaxies and the evolution of L(dust)/L(UV) with the redshift

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• Study of Star-formation in Dual Nuclei Galaxies using UVIT observations
• "Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift
• Multiwavelength study of radio galaxy Pictor A: detection of western hotspot in far-UV and possible origin of high energy emissions
• Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at $z\sim 2.1-3.6$
• Galaxy Rest-Frame UV Colors at z ~ 2-4 with HST UVCANDELS
• SDSS J1059+4251, a highly magnified z ~ 2.8 star-forming galaxy: ESI observations of the rest-frame UV spectrum
• The MOSDEF Survey: Probing Resolved Stellar Populations at $z\sim 2$ Using a New Bayesian-defined Morphology Metric Called Patchiness
• A pilot method to determine the high mass end of the Stellar Initial Mass Function in galaxies using UVIT, H$\alpha$-MUSE observations and applied to NGC628
• GRB 180325A: dust grain-size distribution and interstellar iron nanoparticles contribution
• J-PAS: First Identification, Physical Properties and Ionization Efficiency of Extreme Emission Line Galaxies
• SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars
• Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6
• Non-Parametric Attenuation Curves in Local Star-Forming Galaxies: Geometry Effect, Dust Evolution, and ISS