Star Formation and Dust Attenuation Properties in Galaxies from a Statistical UV-to-FIR Analysis

Abstract

We study two galaxy samples selected in ultraviolet (UV) and in far-infrared (FIR) for which the spectral energy distributions (SEDs) from the far UV (FUV) to the FIR are available. We compare the observed SEDs to modelled SEDs with several star formation histories (SFHs; decaying star formation rate plus burst) and attenuation laws (power law + 2175 Angstroem bump). The Bayesian method allows to estimate statistically the best parameters by comparing each observed SED to the full set of 82800 models. We reach the conclusion that the UV dust attenuation cannot be estimated correctly from an SED analysis if the FIR information is not used. The deduced dispersion is larger than with the FIR data and the distribution is not symetrically distributed about zero: there is an over-estimation for UV-selected galaxies and an under-estimation for FIR-selected galaxies. The output from the analysis process suggests that UV-selected galaxies have attenuation laws in average similar to the LMC extinction while FIR-selected galaxy attenuation laws more resemble the MW extinction law. The dispersion about the average relation in the Log(Fdust/Ffuv) vs. FUV-NUV diagram (once the main relation with FUV-NUV is accounted for) is explained by two other parameters: the slope of the attenuation law and the instantaneous birthrate parameter b_0 for UV-selected galaxies and the same ones plus the strength of the bump for the FIR-selected galaxies. We propose a recipe to estimate the UV dust attenuation for UV-galaxies only (that should be used whenever the FIR information is not available because the resulting Afuv is poorly defined with an uncertainty of about 0.32): A_{FUV} = 1.4168 (FUV-NUV)^2 + 0.3298 (NUV-I)^2 + 2.1207 (FUV-NUV) + 2.7465 (NUV-I) + 5.8408

Accepted for publication in MNRAS, Main Journal

References in corpus (31)

• Star Formation in Galaxies Along the Hubble Sequence
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• Starburst99: Synthesis Models for Galaxies with Active Star Formation
• The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
• Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
• A Simple Model for the Absorption of Starlight by Dust in Galaxies
• The Dependence of Star Formation History and Internal Structure on Stellar Mass for 10^5 Low-Redshift Galaxies
• A Quantitative Comparison of SMC, LMC, and Milky Way UV to NIR Extinction Curves
• Dust Absorption And The Ultraviolet Luminosity Density At z \approx 3 As Calibrated By Local Starburst Galaxies
• The Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry
• The Rest-Frame Optical Properties of z~3 Galaxies
• Dust in the Early Universe: Dust Formation in the Ejecta of Population III Supernovae
• Multiple Scattering in Clumpy Media. II. Galactic Environments
• Dust attenuation in the nearby Universe: comparison between galaxies selected in the ultraviolet or in the infrared
• The infrared side of galaxy formation. I. The local universe in the semi-analytical framework
• The Star Formation Rate of the Universe at z~6 from the Hubble Ultra Deep Field
• Star formation history and dust attenuation in galaxies drawn from ultraviolet surveys
• The UV Galaxy Luminosity Function in the Local Universe from GALEX Data
• Far-Infrared Galaxies in the Far-Ultraviolet
• 1.65mic (H-band) surface photometry of galaxies. VI: The history of star formation in normal late-type galaxies
• New Constraints on the Star Formation Histories and Dust Attenuation of Galaxies in the Local Universe from GALEX
• The Properties of Ultraviolet-Luminous Galaxies at the Current Epoch
• Galaxies at z~7-8: z-dropouts in the Hubble Ultra Deep Field
• A Substantial Population of Red Galaxies at z > 2: Modeling of the Spectral Energy Distributions of an Extended Sample
• Cirrus models for local and high z SCUBA galaxies
• High-Redshift Extremely Red Objects in the HST Ultra Deep Field Revealed by the GOODS IRAC Observations
• Detection of the 2175ÅExtinction Feature at z=0.83
• Dust-Induced Systematic Errors in UV-Derived Star Formation Rates
• Dust emission from the lensed Lyman break galaxy cB58
• Deep mid-infrared observations of Lyman-break galaxies
• GALEX UV Spectroscopy and Deep Imaging of LIRGs in the ELAIS S1 field

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• Blueberry galaxies up to 200 Mpc and their optical and infrared properties
• Discovery of a Very Large (~20 kpc) Galaxy at z=3.72
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
• Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
• Unsupervised classification of CIGALE galaxy spectra
• COSMOS2020: Investigating the AGN-obscured accretion phase at $z\sim 1$ via [NeV] selection
• Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census
• Brackett-$\gamma$ as a Gold-standard Test of Star Formation Rates Derived from SED Fitting
• Accretion History of AGN: Estimating the Host Galaxy Properties in X-ray Luminous AGN from z=0-3
• A Morphological Study on Galaxies Hosting Optical Variability-Selected AGNs in the COSMOS Field
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• Decoding the IRX-β dust attenuation relation in star-forming galaxies at intermediate redshift
• The PAU Survey: galaxy stellar population properties estimates with narrowband data
• The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ~ 5.5
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 $\mu$m and Data Release for the COSMOS Field
• Measuring the Total Ultraviolet Light from Galaxy Clusters at z=0.5-1.6: The Balance of Obscured and Unobscured Star-Formation
• Strong [O III] λ5007 Compact Galaxies Identified from SDSS DR16 and Their Scaling Relations
• RadioSED I: Bayesian inference of radio SEDs from inhomogeneous surveys
• The Lockman-SpReSO project. Description, target selection, observations and preliminary results
• Ionized gas metallicity of the strong [OIII]λ emission-line compact galaxies in the LAMOST survey
• Active galactic nuclei catalog from the AKARI NEP Wide field
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• CEERS: Forging the First Dust Grains in the Universe? A Population of Galaxies with spectroscopically-derived Extremely Low Dust Attenuation (GELDA) at 4.0<z<11.4
• Galaxy Properties Derived with Spectral Energy Distribution Fitting in the Hawaii-Hubble Deep Field-North
• The recent star formation history of NGC 628 on resolved scales
• Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
• Multiple emission lines of H$\alpha$ emitters at $z\sim 2.3$ from the broad and medium-band photometry in the ZFOURGE Survey
• Identifying type II quasars at intermediate redshift with few-shot learning photometric classification
• SIT 45: An interacting, compact, and star-forming isolated galaxy triplet
• SDSS-IV MaNGA: the physical origin of off-galaxy H$\alpha$ blobs in the local Universe
• Far-infrared star-formation rates of six GRB host galaxies with ALMA
• The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Comparing Ultraviolet and Infrared-Selected Starburst Galaxies in Dust Obscuration and Luminosity
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
• On the Thermally Pulsing Asymptotic Giant Branch Contribution to the Light of Nearby Disk Galaxies
• Discovery of Five Green Pea Galaxies with Double-peaked Narrow [OIII] Lines
• A MaNGA view of isolated galaxy mergers in the star-forming Main Sequence
• Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
• VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z\sim 0.15$ traced with VLT/MUSE
• Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups
• Varying linear polarisation in the dust-free GRB 210610B
• ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-ray Detected Active Galactic Nuclei
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Identification of Large Equivalent Width Dusty Galaxies at 4 $<$ z $<$ 6 from Sub-mm Colours
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• Tracing the Total Stellar Mass and Star Formation of High-Redshift Protoclusters
• LBT-MODS spectroscopy of high-redshift candidates in the Chandra J1030 field. A newly discovered z$\sim$2.8 large scale structure
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• Molecular gas in cool-core brightest cluster galaxies at $z\simeq 0.4$
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• The Lockman--SpReSO project. Main properties of infrared selected star-forming galaxies
• Studying Quasar Absorber Host Galaxy Properties Using Image Stacking Technique
• Identification and Properties of Isolated Field Elliptical Galaxies from CFHTLS-W1
• Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
• Near- to mid-infrared spectroscopy of the heavily obscured AGN LEDA 1712304 with AKARI/IRC
• The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
• The Calibration of Polycyclic Aromatic Hydrocarbon Dust Emission as a Star Formation Rate Indicator in the AKARI NEP Survey
• The HI gas fraction scaling relation of the Green Pea galaxies
• Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
• MIRI spectrophotometry of GN-z11: Detection and nature of an optical red continuum component
• Dust contribution to the panchromatic galaxy emission
• The Star Formation History of Redshift z~2 Galaxies: The Role of The Infrared Prior
• The viewing angle in AGN SED models, a data-driven analysis
• HELP project - a dreamed-of multiwavelength dataset for SED fitting: the influence of used models for the main physical properties of galaxies
• AGN in the ULIRG HE 0435-5304
• Overdense fireworks in GOODS-N: Unveiling a record number of massive dusty star forming galaxies at z$\sim$5.2 with the N2CLS
• Connecting the dots: Tracing the evolutionary pathway of Polar Ring Galaxies in the cases of NGC 3718, NGC 2685, and NGC 4262
• Exploring the physical properties of Type II Quasar candidates at intermediate redshifts with CIGALE
• CIGALE: Code Investigating GALaxy Emission
• Molecular gas content and high excitation of a massive main-sequence galaxy at z = 3
• Recovering the properties of the interstellar medium through integrated spectroscopy: application to the z~0 ECO volume-limited star-forming galaxy sample
• The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies
• Ultraviolet-to-far-infra-red self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts
• The major merger-active galactic nucleus connection up to the cosmic noon
• A normalizing flow approach for the inference of star cluster properties from unresolved broadband photometry I: Comparison to spectral energy distribution fitting
• A Lyman continuum analysis for $\sim 100$ galaxies at $z_{\text{spec}}\sim 3$ in the Abell 2744 Cluster Field
• The gMOSS: the galaxy survey and galaxy populations of the large homogeneous field
• GRB 160410A: the first Chemical Study of the Interstellar Medium of a Short GRB
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• A VLT/VIMOS view of two $Planck$ multiple-cluster systems: structure and galaxy properties
• The X-ray statistical properties of dust-obscured galaxies detected by eROSITA
• Mocking IFU observations and metallicity diagnostics from cosmological simulations
• Theoretical clues about dust accumulation and galaxy obscuration at high and low redshift
• The Compact Star-Forming Galaxies at $2<z<3$ in 3D-HST/CANDELS: AGN and Non-AGN Physical Properties
• Warm absorber outflows in radio-loud active galactic nucleus 3C~59
• The Nature of Hyperluminous Infrared Galaxies
• Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
• Investigating the young stellar populations and hierarchies in nearby galaxies with the UVIT. II. Presenting the properties of ~25,000 UV-detected star-forming clumps
• Topological models to infer multiphase interstellar medium properties
• Star formation at z$\sim$0.9 from the OTELO survey: A comprehensive view combining deep optical spectroscopy and infrared data