The Relation Between SFR and Stellar Mass for Galaxies at 3.5 6.5 in CANDELS
arXiv:1407.6012 · doi:10.1088/0004-637X/799/2/183
Abstract
Distant star-forming galaxies show a correlation between their star formation rates (SFR) and stellar masses, and this has deep implications for galaxy formation. Here, we present a study on the evolution of the slope and scatter of the SFR-stellar mass relation for galaxies at using multi-wavelength photometry in GOODS-S from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) and Spitzer Extended Deep Survey. We describe an updated, Bayesian spectral-energy distribution fitting method that incorporates effects of nebular line emission, star formation histories that are constant or rising with time, and different dust attenuation prescriptions (starburst and Small Magellanic Cloud). From =6.5 to =3.5 star-forming galaxies in CANDELS follow a nearly unevolving correlation between stellar mass and SFR that follows SFR with at and at . This evolution requires a star formation history that increases with decreasing redshift (on average, the SFRs of individual galaxies rise with time). The observed scatter in the SFR-stellar mass relation is tight, yr 0.4 dex, for galaxies with dex. Assuming that the SFR is tied to the net gas inflow rate (SFR ), then the scatter in the gas inflow rate is also smaller than 0.30.4 dex for star-forming galaxies in these stellar mass and redshift ranges, at least when averaged over the timescale of star formation. We further show that the implied star formation history of objects selected on the basis of their co-moving number densities is consistent with the evolution in the SFR-stellar mass relation.
arXiv comment31 pages, 24 figures, accepted for publication in ApJ
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- Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25
- An alternate approach to measure specific star formation rates at 2<z<7
- Detection of Lyman-Alpha Emission From a Triple Imaged z=6.85 Galaxy Behind MACS J2129.4-0741
- MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063: II. Properties of low luminosity Lyman alpha emitters at z>3
- ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1<z<4
- An evolving and mass dependent - relation for galaxies
- FirstLight III: Rest-frame UV-optical spectral energy distributions of simulated galaxies at cosmic dawn
- MAGAZ3NE: High Stellar Velocity Dispersions for Ultra-Massive Quiescent Galaxies at
- The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude
- A quasar-galaxy merger at : black hole mass and quasar properties from the NIRSpec spectrum
- Photometric identification and MMT spectroscopy of new extremely metal-poor galaxies: towards a better understanding of young stellar populations at low metallicity
- Properties of five z~0.3-0.4 confirmed LyC leakers: VLT/XShooter observations
- Forward and backward galaxy evolution in comoving number density space
- The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
- The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
- First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
- Texas Spectroscopic Search for Ly Emission at the End of Reionization I. Constraining the Ly Equivalent Width Distribution at 6.0 < < 7.0
- Nebular line emission from z > 7 galaxies in cosmological simulations: rest-frame UV to Optical lines
- RELICS: Spectroscopy of gravitationally-lensed reionization-era analogs and implications for CIII] detections at
- Unbiased Differential Size Evolution and the Inside-Out Growth of Galaxies in the Deep CANDELS GOODS Fields at
- Elevated Hot Gas and High-Mass X-ray Binary Emission in Low Metallicity Galaxies: Implications for Nebular Ionization and Intergalactic Medium Heating in the Early Universe
- Unique Tracks Drive the Scatter of the Spatially-Resolved Star Formation Main Sequence
- The MOSDEF Survey: First Measurement of Nebular Oxygen Abundance at
- Young, Star-forming Galaxies and their local Counterparts: the Evolving Relationship of Mass-SFR-Metallicity since z ~ 2.1
- Possible identification of massive and evolved galaxies At z > 5
- Modelling the M*-SFR relation at high redshift: untangling factors driving biases in the intrinsic scatter measurement
- A census of galaxy constituents in a Coma Progenitor observed at z>3
- RELICS: Properties of z>5.5 Galaxies Inferred from Spitzer and Hubble Imaging Including A Candidate z~6.8 Strong [OIII] Emitter
- A detailed study of massive galaxies in a protocluster at z=3.13
- The relation between star formation rate and stellar mass of galaxies at z 1-4
- The Spitzer/IRAC Legacy over the GOODS Fields: Full-Depth 3.6, 4.5, 5.8 and 8.0um Mosaics and Photometry for > 9000 Galaxies at z~3.5-10 from the GOODS Re-ionization Era wide-Area Treasury from Spitzer (GREATS)
- COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
- An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
- MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3<z<4) from the ZFOURGE Survey
- Spectral Energy Distributions of Companion Galaxies to z6 Quasars
- Texas Spectroscopic Search for Ly Emission at the End of Reionization II. The Deepest Near-Infrared Spectroscopic Observation at
- The impact of the Star Formation Histories on the SFR-M relation at z2
- Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
- Lyman-α Emitters in the context of hierarchical galaxy formation: predictions for VLT/MUSE surveys
- Exploring Photometric Redshifts as an Optimization Problem: An Ensemble MCMC and Simulated Annealing-Driven Template-Fitting Approach
- MCSED: A flexible spectral energy distribution fitting code and its application to emission-line galaxies
- Coevolution of metallicity and star formation in galaxies to z=3.7: II. A theoretical model
- CLEAR: Boosted Ly Transmission of the Intergalactic Medium in UV bright Galaxies
- (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies IV. Physical properties derived from spectral energy distributions
- ZFOURGE: Extreme 5007 emission may be a common early-lifetime phase for star-forming galaxies at
- Differences and similarities of stellar populations in LAEs and LBGs at 3.4 - 6.8
- The rapid transition from star-formation to AGN dominated rest-frame UV light at z ~ 4
- The relation between morphology, star formation history, and environment in local universe galaxies
- The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
- UV regulated star formation in high-redshift galaxies
- Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
- Dust attenuation of the nebular regions and optical emission lines of star-forming galaxies
- Bayesian hierarchical modelling of the -SFR relation from 1<z<6 in ASTRODEEP
- SHARDS: A global view of the star formation activity at z~0.84 and z~1.23
- The dominance of quenching through cosmic times
- Probing the Physical Properties of z=4.5 Lyman Alpha Emitters with Spitzer
- Probing the Star Formation Main Sequence down to M at
- The Complete Local Volume Groups Sample -- IV. Star formation and gas content in group-dominant galaxies
- Clustering dependence on Lyman- luminosity from MUSE surveys at
- The FMOS-COSMOS survey of star-forming galaxies at . V: Properties of dark matter halos containing H emitting galaxies
- ISM conditions in z~0.2 Lyman-Break Analogs
- J-PLUS: The star formation main sequence and rate density at d < 75 Mpc
- The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
- How the super-Eddington regime affects black hole spin evolution in high-redshift galaxies
- Spectroscopy of CASSOWARY gravitationally-lensed galaxies in SDSS: characterisation of an extremely bright reionization-era analog at
- Correlations between H Equivalent Width and Galaxy Properties at : Physical or Selection-driven?
- FirstLight IV: Diversity in sub-L galaxies at cosmic dawn
- Deep Spitzer/IRAC Data for z~10 galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ~500 Myr of Cosmic Time
- The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence
- The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at with CO stacking of MUSE detected Galaxies
- MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
- A [C II] 158m Emitter Associated with an OI Absorber at the End of the Reionization Epoch
- The high-redshift Universe with Spitzer
- A spectroscopic study of a rich cluster at z=1.52 with Subaru LBT: the environmental impacts on the mass-metallicity relation
- Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
- Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
- Starburst galaxies in semi-analytic models of galaxy formation and evolution
- MAGAZ3NE: Massive, Extremely Dusty Galaxies at Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at
- A model for the infrared-radio correlation of main-sequence galaxies at GHz frequencies and its variation on redshift and stellar mass
- The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
- A selection of Hα emitters at z = 2.1-2.5 using the Ks-band photometry of ZFOURGE
- The star-forming main sequence and the contribution of dust-obscured star formation since from the FUV+IR luminosity functions
- The Ultraviolet Deep Imaging Survey of Galaxies in the Bootes Void I: catalog, color-magnitude relations and star formation
- Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
- Effect of the environment on star formation activity and stellar mass for star-forming galaxies in the COSMOS field
- ALMA 1.1mm Observations of a Conservative Sample of High Redshift Massive Quiescent Galaxies in SHELA
- Exploring the evolution of star formation and dwarf galaxy properties with JWST/MIRI serendipitous spectroscopic surveys
- Gamma-Ray Burst Host Galaxies: Specific Star Formation Rate vs. Metallicity
- COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at
- Predicting the intensity mapping signal for multi- CO lines
- Star-formation-rate estimates from water emission
- Bridging between the integrated and resolved main sequence of star formation
- The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at
- What halts the growth of galaxies?
- The MUSE Hubble Ultra Deep Field Survey XIV. The evolution of the Lya emitter fraction from z=3 to z=6
- Sub-Gyr variability around the SFMS and its contribution to the scatter
- The VIMOS Public Extragalactic Redshift Survey (VIPERS). The complexity of galaxy populations at 0.4< z<1.3 revealed with unsupervised machine-learning algorithms
- Main sequence of star formation and colour bimodality considering galaxy environment
- The Nature of Hyperluminous Infrared Galaxies
- The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
- The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5