On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3

Abstract

We compare multi-wavelength SFR indicators out to z~3 in GOODS-South. Our analysis uniquely combines U-to-8um photometry from FIREWORKS, MIPS 24um and PACS 70, 100, and 160um photometry from the PEP survey, and Ha spectroscopy from the SINS survey. We describe a set of conversions that lead to a continuity across SFR indicators. A luminosity-independent conversion from 24um to total infrared luminosity yields estimates of LIR that are in the median consistent with the LIR derived from PACS photometry, albeit with significant scatter. Dust correction methods perform well at low to intermediate levels of star formation. They fail to recover the total amount of star formation in systems with large SFR_IR/SFR_UV ratios, typically occuring at the highest SFRs (SFR_UV+IR \gtrsim 100 Msun/yr) and redshifts (z \gtrsim 2.5) probed. Finally, we confirm that Ha-based SFRs at 1.5<z<2.6 are consistent with SFR_SED and SFR_UV+IR provided extra attenuation towards HII regions is taken into account (Av,neb = Av,continuum / 0.44). With the cross-calibrated SFR indicators in hand, we perform a consistency check on the star formation histories inferred from SED modeling. We compare the observed SFR-M relations and mass functions at a range of redshifts to equivalents that are computed by evolving lower redshift galaxies backwards in time. We find evidence for underestimated stellar ages when no stringent constraints on formation epoch are applied. We demonstrate how resolved SED modeling, or alternatively deep UV data, may help to overcome this bias. The age bias is most severe for galaxies with young stellar populations, and reduces towards older systems. Finally, our analysis suggests that SFHs typically vary on timescales that are long (at least several 100 Myr) compared to the galaxies' dynamical time.

Accepted for publication in The Astrophysical Journal, 19 pages, 15 figures

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• A Uniform History for Galaxy Evolution
• A ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259
• Spatially resolved star formation and dust attenuation in Mrk848: Comparison of the integral field spectra and the UV-to-IR SED
• Estimating dust attenuation from galactic spectra. II. Stellar and gas attenuation in star-forming and diffuse ionized gas regions in MaNGA
• On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELS
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• HI galaxies with little star formation: an abundance of LIERs
• Compact molecular gas emission in local LIRGs among low- and high-z galaxies
• Star formation and AGN activity in the most luminous LINERs in the local universe
• Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
• Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates
• Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since $z\sim 0.7$
• Dust attenuation of the nebular regions and optical emission lines of $z\sim 2$ star-forming galaxies
• The UV to FIR spectral energy distribution of star-forming galaxies in the redshift desert
• Star formation in far-IR AGN and non-AGN galaxies in the green valley. II. Morphological analysis
• The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV & [OII]λ3727 luminosities
• Galaxy morphologies at cosmic noon with JWST: A foundation for exploring gas transport with bars and spiral arms
• Sacrificing information for the greater good: how to select photometric bands for optimal accuracy
• The physical properties of local (U)LIRGs: a comparison with nearby early- and late-type galaxies
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• SXDF-ALMA 2 Arcmin^2 Deep Survey: Resolving and Characterizing the Infrared Extragalactic Background Light Down to 0.5 mJy
• Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S Field
• The whole picture of the large-scale structure of the CL1604 supercluster at z$\sim$0.9
• De-Confusing blended field images using graphs and bayesian priors
• Variation of the Nebular Dust Attenuation Curve with the Properties of Local Star-forming Galaxies
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Euclid preparation. XXX. Performance assessment of the NISP Red-Grism through spectroscopic simulations for the Wide and Deep surveys
• Optical-faint, Far-infrared-bright Herschel Sources in the CANDELS Fields: Ultra-Luminous Infrared Galaxies at z>1 and the Effect of Source Blending
• Host galaxy properties and environment of obscured and unobscured X-ray selected Active Galactic Nuclei in the COSMOS survey
• HST viewing of spectacular star-forming trails behind ESO 137-001
• Listening to galaxies tuning at z ~ 2.5 - 3.0: The first strikes of the Hubble fork
• The star-forming progenitors of massive red galaxies
• Panchromatic Estimation of Star Formation Rates in BzK Galaxies at 1<z<3
• Herschel observations of a z~2 stellar mass selected galaxy sample drawn from the GOODS NICMOS Survey
• Differential attenuation in star-forming galaxies at 0.3 $\lesssim$ $z$ $\lesssim$ 1.5 in the SHARDS/CANDELS field
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• No evidence for feedback: Unexceptional Low-ionization winds in Host galaxies of Low Luminosity Active Galactic Nuclei at Redshift z ~1
• First Light And Reionisation Epoch Simulations (FLARES) XII: The consequences of star-dust geometry on galaxies in the EoR
• A Variant Stellar-to-nebular Dust Attenuation Ratio on Subgalactic and Galactic Scales
• Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
• Bulgeless galaxies in the COSMOS field: environment and star formation evolution at $z<1$
• The mass dependence of structure, star formation rate, and mass assembly mode at 0.5<z< 2.5
• A Universal Relation of Dust Obscuration Across Cosmic Time
• A deeper look at the dust attenuation law of star-forming galaxies at high redshift
• On the Evolution of the Bi-Modal Distribution of Galaxies in the Plane of Specific Star Formation Rate versus Stellar Mass
• Structures, stellar population properties, AGN fractions, and environments of massive compact galaxies at $1<z<2$ in 3D--{\it HST}/CANDELS
• Revisiting the Color-Color Selection: Submillimeter and AGN Properties of NUV-r-J Selected Quiescent Galaxies
• Starbursts and High-Redshift Galaxies are Radioactive: High Abundances of ${}^{26}$Al and Other Short Lived Radionuclides
• The physical properties of massive green valley galaxies as a function of environments at $0.5<z<2.5$ in 3D-\textit{HST}/CANDELS fields
• Physical Properties of the Host Galaxies of Ca-rich Transients
• The effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
• The MOSDEF Survey: The Dependence of H$\alpha$-to-UV SFR Ratios on SFR and Size at $z\sim 2$
• Dust correction factors over $0<z<3$ in massive star-forming galaxies from stacking in \emph{Herschel}
• The MOSDEF Survey: Calibrating the relationship between H$\alpha$ star-formation rate and radio continuum luminosity at $1.4<z<2.6$
• The Role of Bulge Formation in the Homogenization of Stellar Populations at $z\sim 2$ as revealed by Internal Color Dispersion in CANDELS
• Exploring the Correlation between $\mathrm{H}\alpha$-to-UV Ratio and Burstiness for Typical Star-forming Galaxies at $z\sim 2$
• MusE GAs FLOw and Wind (MEGAFLOW) VII. A NOEMA pilot program to probe molecular gas in galaxies with measured circumgalactic gas flows
• Insights from Synthetic Star-forming Regions: III. Calibration of Measurement Techniques of Star-formation Rates
• Insights on star formation histories and physical properties of $1.2\le z\lesssim 4$ Herschel-detected galaxies
• CO Multi-line Imaging of Nearby Galaxies (COMING). X. Physical conditions of molecular gas and the local SFR-Mass relation
• COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
• Bursting and quenching in satellite galaxies
• Brackett-$\gamma$ as a Gold-standard Test of Star Formation Rates Derived from SED Fitting
• A Method to improve line flux and redshift measurements with narrowband filters
• A magnified view of star formation at redshift 0.9 from two lensed galaxies
• High dense gas fraction in a gas-rich star-forming galaxy at z = 1.2
• Star formation in LINER host galaxies at z~0.3
• Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators
• SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139
• Photometric Redshifts of Submillimeter Galaxies
• KMTNet Nearby Galaxy Survey III. Deficient H$\alpha$ flux in the Extended Disks of Spiral Galaxies
• The SCUBA-2 Cosmology Legacy Survey: The EGS deep field -- III. The evolution of faint submillimeter galaxies at $z<4$
• How accurate are infrared luminosities from monochromatic photometric extrapolation?
• Understanding the Universal Dust Attenuation Scaling Relation of Star-Forming Galaxies
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• H$\alpha$-based Star Formation Rates in and around z $\sim$ 0.5 EDisCS clusters
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
• Star formation history of $0.1\le \text{z}\le 1.5$ mass-selected galaxies in the ELAIS-N1 Field
• Are the hosts of VLBI selected radio-AGN different to those of radio-loud AGN?
• Central star formation in double-peak gas rich radio galaxies
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• Predicting HCN, HCO${}^{+}$, multi-transition CO, and dust emission of star-forming galaxies -- Extension to luminous infrared galaxies and the role of cosmic ray ionization
• The effect of environment on the properties of the most massive galaxies at $0.5<z<2.5$ in the cosmos-dash field
• The MOSDEF Survey: Probing Resolved Stellar Populations at $z\sim 2$ Using a New Bayesian-defined Morphology Metric Called Patchiness
• Evolutionary synthesis models as a tool and guide towards the first galaxies
• Quantifying the effect of field variance on the H$\alpha$ luminosity function with the New Numerical Galaxy Catalogue (${\nu }^2$GC)
• Measuring the gas reservoirs in $10^8<$ M${}_{\star }<10^{11}$ M${}_{\odot }$ galaxies at $1\le z\le 3$
• Evolved galaxies in high-density environments across $2.0\le z<4.2$ using the ZFOURGE survey
• A first look at a complete view of spatially resolved star formation at 1<z<1.8 with JWST NGDEEP+FRESCO slitless spectroscopy
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• Structural and morphological properties of ultraluminous infrared galaxies at $1<z<3$
• The Compact Star-Forming Galaxies at $2<z<3$ in 3D-HST/CANDELS: AGN and Non-AGN Physical Properties
• Far-infrared observations of dust in Ly$\alpha$ emitters at z=2-6
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution