The SFR-M* Relation and Empirical Star-Formation Histories from ZFOURGE at 0.5 < z < 4

Abstract

We explore star-formation histories (SFHs) of galaxies based on the evolution of the star-formation rate stellar mass relation (SFR-M*). Using data from the FourStar Galaxy Evolution Survey (ZFOURGE) in combination with far-IR imaging from the Spitzer and Herschel observatories we measure the SFR-M* relation at 0.5 < z < 4. Similar to recent works we find that the average infrared SEDs of galaxies are roughly consistent with a single infrared template across a broad range of redshifts and stellar masses, with evidence for only weak deviations. We find that the SFR-M* relation is not consistent with a single power-law of the form SFR ~ M*^a at any redshift; it has a power-law slope of a~1 at low masses, and becomes shallower above a turnover mass (M_0) that ranges from 10^9.5 - 10^10.8 Msol, with evidence that M_0 increases with redshift. We compare our measurements to results from state-of-the-art cosmological simulations, and find general agreement in the slope of the SFR-M* relation albeit with systematic offsets. We use the evolving SFR-M* sequence to generate SFHs, finding that typical SFRs of individual galaxies rise at early times and decline after reaching a peak. This peak occurs earlier for more massive galaxies. We integrate these SFHs to generate mass-growth histories and compare to the implied mass-growth from the evolution of the stellar mass function. We find that these two estimates are in broad qualitative agreement, but that there is room for improvement at a more detailed level. At early times the SFHs suggest mass-growth rates that are as much as 10x higher than inferred from the stellar mass function. However, at later times the SFHs under-predict the inferred evolution, as is expected in the case of additional growth due to mergers.

arXiv commentAccepted for publication in the ApJ: 16 pages, 11 figures, 1 table

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• Evolution of thermal and nonthermal radio continuum emission on kpc scales--Predictions for SKA
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Gas Accretion and Star-Formation Rates with IFUs and Background Quasars
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Star formation history of $0.1\le \text{z}\le 1.5$ mass-selected galaxies in the ELAIS-N1 Field
• Unveiling the gravitationally unstable disc of a massive star-forming galaxy using NOEMA and MUSE
• The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z $\sim$ 4.4-5.9
• Cosmology with One Galaxy: Auto-Encoding the Galaxy Properties Manifold
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at $3<z<4$
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
• Evolved galaxies in high-density environments across $2.0\le z<4.2$ using the ZFOURGE survey
• The effects of star formation history in the SFR-M relation of HII galaxies
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• AGN in the ULIRG HE 0435-5304
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Measuring the gas reservoirs in $10^8<$ M${}_{\star }<10^{11}$ M${}_{\odot }$ galaxies at $1\le z\le 3$
• Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
• The Physical Properties of Star-Forming Galaxies with Strong [O III] Lines at z=3.25
• The metallicity dependence of long-duration gamma-ray bursts
• Main sequence of star formation and colour bimodality considering galaxy environment
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• What halts the growth of galaxies?
• The cosmic environment overtakes the local density in shaping galaxy star formation
• Deep Learning for Galaxy Mergers in the Galaxy Main Sequence
• Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
• Low star-formation activity and low gas content of quiescent galaxies at $z=$ 3.5-4.0 constrained with ALMA
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies