Dust-Corrected Star Formation Rates of Galaxies. II. Combinations of Ultraviolet and Infrared Tracers

Abstract

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total infrared to FUV luminosity ratio (IRX) and the FUV-NUV color. We find that the IRX-corrected FUV luminosities are tightly and linearly correlated with the attenuation-corrected Hα luminosities (as measured from the Balmer decrement), with a rms scatter of $\pm 0.09$ dex. The ratios of these attenuation-corrected FUV to Hα luminosities are consistent with evolutionary synthesis model predictions, assuming a constant star formation rate over 100 Myr, solar metallicity and either a Salpeter or a Kroupa IMF with lower and upper mass limits of 0.1 and 100\msun. The IRX-corrected FUV to Balmer-corrected Hα luminosity ratios do not show any trend with other galactic properties over the ranges covered by our sample objects. In contrast, FUV attenuation derived from the FUV-NUV color (UV spectral slope) show much larger random and systematic uncertainties. When compared to either Balmer-corrected Hα luminosities or IRX-corrected FUV luminosities the color-corrected FUV luminosities show $\sim 2.5$ times larger rms scatter, and systematic nonlinear deviations as functions of luminosity and other parameters. Linear combinations of 25um and 1.4GHz radio continuum luminosities with the observed FUV luminosities are also well correlated with the Balmer-corrected Hα luminosities. These results provide useful prescriptions for deriving attenuation-corrected star formation rates of galaxies based on linear combinations of UV and IR or radio luminosities, which are presented in convenient tabular form. Comparisons of our calibrations with attenuation corrections in the literature and with dust attenuation laws are also made.

54 pages, 16 figures, accepted for publication in The Astrophysical Journal

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• Cold HI in faint dwarf galaxies
• SUPER VII. Morphology and kinematics of H$\alpha$ emission in AGN host galaxies at Cosmic noon using SINFONI
• The MOSDEF Survey: No Significant Enhancement in Star Formation or Deficit in Metallicity in Merging Galaxy Pairs at 1.5<=z<=3.5
• Star Formation Histories Across the Interacting Galaxy NGC 6872, the Largest-Known Spiral
• Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past
• A Big Red Dot: Scattered light, host galaxy signatures and multi-phase gas flows in a luminous, heavily reddened quasar at cosmic noon
• The MOSDEF Survey: Differences in SFR and Metallicity for Morphologically-Selected Mergers at z~2
• A comprehensive X-ray and multiwavelength study of the Colliding Galaxy Pair NGC2207/IC2163
• Variation of the Nebular Dust Attenuation Curve with the Properties of Local Star-forming Galaxies
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at $z\sim 4.5$ with [OII] and [CII] Line Emission $-$ ISM Properties and [OII]$-$SFR Relation
• The Ultraviolet and Infrared Star Formation Rates of Compact Group Galaxies: An Expanded Sample
• Evidence for galaxy quenching in the green valley caused by a lack of a circumgalactic medium
• Apertif view of the OH Megamaser IRAS 10597+5926: OH 18 cm satellite lines in wide-area HI surveys
• The cold interstellar medium of a normal sub-$L^{\star }$ galaxy at the end of reionization
• Hα to FUV ratios in resolved star forming region populations of nearby spiral galaxies
• Characterizing Ultraviolet and Infrared Observational Properties for Galaxies. II. Features of Attenuation Law
• Direct-method metallicity gradients derived from spectral stacking with SDSS-IV MaNGA
• HST viewing of spectacular star-forming trails behind ESO 137-001
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• JWST and ALMA discern the assembly of structural and obscured components in a high-redshift starburst galaxy
• Probing star formation in galaxies at $z\approx 1$ via a Giant Metrewave Radio Telescope stacking analysis
• The Panchromatic Hubble Andromeda Treasury. VI. The reliability of far-ultraviolet flux as a star formation tracer on sub-kpc scales
• The Panchromatic Hubble Andromeda Treasury XVII. Examining Obscured Star Formation with Synthetic Ultraviolet Flux Maps in M31
• The Lyman Alpha Reference Sample XI: Efficient Turbulence Driven Lyα Escape and the Analysis of IR, CO and [C II]158 μm
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• On the Impact of Inclination-Dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• The Evolution of the Far-UV Luminosity Function and Star Formation Rate Density of the Chandra Deep Field South from z=0.2-1.2 with Swift/UVOT
• MaNGA 8313-1901: gas accretion observed in a blue compact dwarf galaxy?
• Far-Ultraviolet and Far-Infrared Bivariate Luminosity Function of Galaxies: Complex Relation between Stellar and Dust Emission
• Spatially-resolved Stellar Population Properties of the M 51-NGC 5195 System from Multi-wavelength Photometric Data
• The cold molecular gas in z$\gtrsim$6 quasar host galaxies
• The UV spectral slope beta and stellar population of most active star-forming galaxies at z~4
• The average submillimetre properties of Lyman-alpha Blobs at z=3
• Gas dynamics and star formation in NGC 6822
• The SFR-radius connection: data and implications for wind strength and halo concentration
• The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope
• Heating and cooling of the neutral ISM in the NGC4736 circumnuclear ring
• Galaxies of the $z\sim 2$ Universe. I. Grism-Selected Rest-Frame Optical Emission Line Galaxies
• Star formation in outer rings of S0 galaxies. I. NGC 6534 and MCG 11-22-015
• Multiwavelength Scrutiny of X-ray Sources in Dwarf Galaxies: ULXs versus AGN
• New-generation dust emission templates for star-forming galaxies
• The cooler past of the intracluster medium in TNG-Cluster
• Getting ready for the LSST data -- estimating the physical properties of $z<2.5$ main sequence galaxies
• The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223
• Star-formation rate in compact star-forming galaxies
• A Method to Extract Spatially Resolved Polycyclic Aromatic Hydrocarbon Emission from Spitzer Spectra: Application to M51
• Halpha imaging survey of Wolf-Rayet galaxies: morphologies and star formation rates
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Rotational Dynamics and Star Formation in the Nearby Dwarf Galaxy NGC 5238
• The MOSDEF Survey: Calibrating the relationship between H$\alpha$ star-formation rate and radio continuum luminosity at $1.4<z<2.6$
• Dust Buried Compact Sources in the Dwarf Galaxy NGC 4449
• Exploring X-ray Binary Populations in Compact Group Galaxies with $Chandra$
• The MOSDEF Survey: The Dependence of H$\alpha$-to-UV SFR Ratios on SFR and Size at $z\sim 2$
• Cold gas mass measurements for the era of large optical spectroscopic surveys
• A panchromatic view of star cluster formation in a simulated dwarf galaxy starburst
• The metallicity evolution of blue compact dwarf galaxies from the intermediate redshift to the local Universe
• Inside-out growth or inside-out quenching? clues from colour gradients of local galaxies
• A study on the Clustering Properties of Radio-Selected sources in the Lockman Hole Region at 325 MHz
• Near-identical star formation rate densities from H$\alpha$ and FUV at redshift zero
• Massive star formation in galaxies with excess UV emission
• Decoding the IRX-β dust attenuation relation in star-forming galaxies at intermediate redshift
• Starbursting Brightest Cluster Galaxy: a Herschel view of the massive cluster MACS J1931.8-2634
• The impact of low luminosity AGN on their host galaxies: A radio and optical investigation of the kpc-scale outflow in MaNGA 1-166919
• A Multi-Wavelength Study of Star Formation in 15 Local Star-Forming Galaxies
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• An uncertainty principle for star formation -- V. The influence of dust extinction on star formation rate tracer lifetimes and the inferred molecular cloud lifecycle
• The JWST Emission Line Survey (JELS): Extending rest-optical narrow-band emission line selection into the Epoch of Reionization
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• On recent SFR calibrations and the constant SFR approximation
• Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
• The spatially-resolved correlation between [NII] 205 μm line emission and the 24 μm continuum in nearby galaxies
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• OMEGA - OSIRIS Mapping of Emission-line Galaxies in A901/2: IV. - Extinction of Star-Formation Estimators with Inclination
• The influence of galaxy surface brightness on the mass-metallicity relation
• Improved method to determine the integrated properties of nuclear rings: NGC 1512
• Polycyclic aromatic hydrocarbon excitation in nearby spiral galaxies
• Spatial Correlation Between Dust and H$\alpha$ Emission in Dwarf Irregular Galaxies
• The Ultraviolet Deep Imaging Survey of Galaxies in the Bootes Void I: catalog, color-magnitude relations and star formation
• The truncation of the disk of NGC 4565: Detected up to z=4 kpc, with star formation, and affected by the warp
• The dependence of the IR-radio correlation on the metallicity
• Environmental effects in Herschel observations of the ionized carbon content of star forming dwarf galaxies in the Virgo cluster
• Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
• The H$\alpha$ and [O III] $\lambda 5007$ Luminosity Functions of $1.2<z<1.9$ Emission-Line Galaxies from HST Grism Spectroscopy
• SCUSS u-Band Emission as a Star-Formation-Rate Indicator
• A comparison of young star properties with local galactic environment for LEGUS/LITTLE THINGS dwarf irregular galaxies
• Are superthin galaxies low surface brightness galaxies seen edge-on? The star formation probe
• The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). VI: The UV luminosity function of the Virgo cluster and its surrounding regions
• Star formation in the centre of NGC 1808 as observed by ALMA
• Extragalactic Gamma-ray Background from Star-forming Galaxies: Will Empirical Scalings Suffice?
• Star Formation and Dust Extinction Properties of Local Galaxies as seen from AKARI and GALEX
• EIG - II. Intriguing characteristics of the most extremely isolated galaxies
• Understanding the Universal Dust Attenuation Scaling Relation of Star-Forming Galaxies
• Properties of galaxies at the faint end of the H$\alpha$ luminosity function at $z\sim 0.62$
• CO Excitation in High-z Main Sequence Analogues: Resolved CO(4-3)/CO(3-2) Line Ratios in DYNAMO Galaxies
• The disk averaged star formation relation for Local Volume dwarf galaxies
• One of Everything: The Breakthrough Listen Exotica Catalog
• Star formation drivers across the M33 disk
• The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)
• Study of Star-formation in Dual Nuclei Galaxies using UVIT observations
• SDSS-IV MaNGA: Ionization sources of diffuse extra-planar galactic medium
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• X-ray Properties of Optically Variable Low-mass AGN Candidates
• Disentangling emission from star-forming regions in the Magellanic Clouds: Linking [OIII]88 micron and 24 micron
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• The MOSDEF Survey: Probing Resolved Stellar Populations at $z\sim 2$ Using a New Bayesian-defined Morphology Metric Called Patchiness
• Tracing Embedded Stellar Populations in Clusters and Galaxies using Molecular Emission: Methanol as a Signature of the Low-Mass End of the IMF
• The Volumetric Extended-Schmidt Law: A Unity Slope
• The Cold Dust Content of the Nearby Galaxies IC 5325, NGC 7496, NGC 7590, and NGC 7599
• The Lockman--SpReSO project. Main properties of infrared selected star-forming galaxies
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• Northern Galactic Molecular Cloud Clumps in Hi-GAL: Clump and Star Formation within Clouds
• A PAH deficit in the starburst core of a distant spiral galaxy
• 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
• The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
• Interpreting Millimeter Emission from IMEGIN galaxies NGC 2146 and NGC 2976
• The HI gas fraction scaling relation of the Green Pea galaxies
• Star formation and gas in the minor merger UGC 10214
• GMRT H I mapping of mid-infrared bright Blue Compact Dwarf Galaxies W1016+3754 & W2326+0608
• Searching for the magnetised Tidal Dwarf Galaxies in Hickson Compact Groups: HCG 26, 91, and 96
• Dashing through the cluster: An X-ray to radio view of UGC 10420 undergoing ram-pressure stripping
• Narrowband H$\alpha$ imaging of nearby Wolf-Rayet galaxies
• AstroSat observations of interacting galaxies NGC 7469 and IC 5283
• What goes around comes around: the fate of stars in stripped tails of gas
• ALMA Lensing Cluster Survey: average dust, gas, and star formation properties of cluster and field galaxies from stacking analysis
• Investigating Galactic Fountains in M101: Insights from Ionized, UV emissions and Neutral Gas
• Cluster environment quenches the star formation of low-mass satellite galaxies from the inside-out
• On the origin of the anomalous gas, non-declining rotation curve and disc asymmetries in NGC253
• SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
• Probing star formation and ISM properties using galaxy disk inclination II: Testing typical FUV attenuation corrections out to z$\sim$0.7
• Wandering Black Hole Candidates in Dwarf Galaxies at VLBI Resolution
• Extended H$\alpha$ over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at $z\sim 2$
• Dust and inclination corrected star-formation and interstellar medium scaling relations in nearby galaxies
• Searching Far and Long I: Pilot ALMA 2mm Follow-up of Bright Dusty Galaxies as a Redshift Filter
• Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim 1.74$ MaDCoWS2 galaxy cluster candidate
• Estimating Galaxy Star Formation Rates from Murchison Widefield Array Radio Continuum Emission
• ESO 137-002: a large spiral undergoing edge-on ram-pressure stripping with little star formation in the tail
• 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
• Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
• PHANGS-MUSE: the HII region luminosity function of local star-forming galaxies
• Spatially-resolved analysis of neutral winds, stars and ionized gas kinematics with MEGARA/GTC: new insights on the nearby galaxy UGC 10205
• Global Hot Gas Excess in (U)LIRGs: Replicating Galactic Nuclei Scaling Relations between Diffuse X-ray Emission and Star Formation on Galaxy-Wide Scales