Young, Star-forming Galaxies and their local Counterparts: the Evolving Relationship of Mass-SFR-Metallicity since z ~ 2.1
arXiv:1511.08243 · doi:10.3847/0004-637X/817/1/10
Abstract
We explore the evolution of the Stellar Mass-Star Formation Rate-Metallicity Relation using a set of 256 COSMOS and GOODS galaxies in the redshift range 1.90 < z < 2.35. We present the galaxies' rest-frame optical emission-line fluxes derived from IR-grism spectroscopy with the Hubble Space Telescope and combine these data with star formation rates and stellar masses obtained from deep, multi-wavelength (rest-frame UV to IR) photometry. We then compare these measurements to those for a local sample of galaxies carefully matched in stellar mass (7.5 < log(M*/Msol) < 10.5) and star formation rate (-0.5 < log(SFR) < 2.5 in Msol yr^-1). We find that the distribution of z ~ 2.1 galaxies in stellar mass-SFR-metallicity space is clearly different from that derived for our sample of similarly bright (L_H\b{eta} > 3 . 10^40 ergs s^-1) local galaxies, and this offset cannot be explained by simple systematic offsets in the derived quantities. At stellar masses above ~10^9 Msol and star formation rates above ~10 Msol yr^-1, the z ~ 2.1 galaxies have higher oxygen abundances than their local counterparts, while the opposite is true for lower-mass, lower-SFR systems.
References in corpus (20)
- Cosmic Star Formation History
- The Cosmic Evolution Survey (COSMOS) -- Overview
- The Mass-Metallicity Relation at z~2
- 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
- Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
- Strong Nebular Line Ratios in the Spectra of z~2-3 Star-forming Galaxies: First Results from KBSS-MOSFIRE
- H-alpha Observations of a Large Sample of Galaxies at z~2: Implications for Star Formation in High Redshift Galaxies
- The Relation Between SFR and Stellar Mass for Galaxies at 3.5 6.5 in CANDELS
- The MOSDEF Survey: Mass, Metallicity, and Star-formation Rate at z~2.3
- New insights into the stellar content and physical conditions of star-forming galaxies at z = 2-3 from spectral modelling
- The MOSDEF Survey: Excitation Properties of Star-forming Galaxies
- AGN Emission Line Diagnostics and the Mass-Metallicity Relation up to Redshift z~2: the Impact of Selection Effects and Evolution
- The MOSDEF Survey: Optical AGN Diagnostics at z~2.3
- A Consistent Study of Metallicity Evolution at 0.8 < z < 2.6
- The HETDEX Pilot Survey V: The Physical Origin of Lyman-alpha Emitters Probed by Near-infrared Spectroscopy
- The mass-metallicity and fundamental metallicity relations at z>2 using VLT and Subaru near-infrared spectroscopy of zCOSMOS galaxies
- Dust Attenuation in High Redshift Galaxies -- 'Diamonds in the Sky'
- Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lyman-alpha Emitters in COSMOS and GOODS-N
- The Relationship between Stellar Mass, Gas Metallicity, and Star Formation Rate for Halpha-selected Galaxies at z~0.8 from the NewHalpha Survey
- 3D-HST Emission Line Galaxies at z ~ 2: Discrepancies in the Optical/UV Star Formation Rates
Cited by in corpus (26)
- De Re Metallica: The cosmic chemical evolution of galaxies
- The Mass-Metallicity and the Fundamental Metallicity Relation revisited on a fully Te-based abundance scale for galaxies
- The MOSDEF Survey: The Evolution of the Mass-Metallicity Relation from to
- MUFASA: Galaxy star formation, gas, and metal properties across cosmic time
- The MOSDEF survey: a stellar mass-SFR-metallicity relation exists at
- Galaxy metallicity scaling relations in the EAGLE simulations
- Fundamental metallicity relation in CALIFA, SDSS-IV MaNGA and high-z galaxies
- Merger-Induced Metallicity Dilution in Cosmological Galaxy Formation Simulations
- Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at 2
- Stellar Mass--Gas-phase Metallicity Relation at : A Power Law with Increasing Scatter toward the Low-mass Regime
- The mass-metallicity relation at z~1-2 and its dependence on star formation rate
- Galaxy pairs in the Sloan Digital Sky Survey -- XIV. Galaxy mergers do not lie on the Fundamental Metallicity Relation
- Direct T metallicity calibration of R23 in strong line emitters
- Neptune long-lived atmospheric features in 2013-2015 from small (28-cm) to large (10-m) telescopes
- Coevolution of metallicity and star formation in galaxies to z=3.7: II. A theoretical model
- Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
- Gas Accretion and Galactic Chemical Evolution: Theory and Observations
- Unravelling the Dust Attenuation Scaling Relations and their Evolution
- Galaxies of the Universe. I. Grism-Selected Rest-Frame Optical Emission Line Galaxies
- HETDEX [OIII] Emitters I: A spectroscopically selected low-redshift population of low-mass, low-metallicity galaxies
- Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
- HETDEX Pilot Survey. VI. [OIII] Emitters and Expectations for a Local Sample of Star Forming Galaxies in HETDEX
- Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
- Revisiting the Local Star-Forming Galaxies Observed in the HETDEX Pilot Survey
- Disentangling AGN and Star Formation Activity at High Redshift Using Hubble Space Telescope Grism Spectroscopy
- Re-examining the Bayesian colour excess estimation for the local star-forming galaxies observed in the HETDEX Pilot Survey