The Evolution of the Global Stellar Mass Density at 0 < z < 3

Abstract

The build-up of stellar mass in galaxies is the consequence of their past star formation and merging histories. Here we report measurements of rest-frame optical light and calculations of stellar mass at high redshift based on an infrared-selected sample of galaxies from the Hubble Deep Field North. The bright envelope of rest-frame B-band galaxy luminosities is similar from 0<z<3, and the co-moving luminosity density is constant to within a factor of 3 over that redshift range. However, galaxies at higher redshifts are bluer, and stellar population modeling indicates that they had significantly lower mass-to-light ratios than those of present-day L* galaxies. This leads to a global stellar mass density, Omega_*(z), which rises with time from z=3 to the present. This measurement essentially traces the integral of the cosmic star formation history that has been the subject of previous investigations. 50-75% of the present-day stellar mass density had formed by z ~ 1, but at z ~= 2.7 we find only 3-14% of today's stars were present. This increase in Omega_* with time is broadly consistent with observations of the evolving global star formation rate once dust extinction is taken into account, but is steeper at 1<z<3 than predicted by some recent semi-analytic models of galaxy formation. The observations appear to be inconsistent with scenarios in which the bulk of stars in present-day galactic spheroids formed at z>>2.

To appear in the Astrophysical Journal. 35 pages, 8 figures, some in color

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• A Link to the Past: Using Markov Chain Monte Carlo Fitting to Constrain Fundamental Parameters of High-Redshift Galaxies
• Passive and star-forming galaxies at $1.4\le z\le 2.5$ in the Aegis field
• Observational signature of circumstellar interaction and ${}^{56}$Ni-mixing in the Type II Supernova 2016gfy
• Cosmic evolution of metal densities: the enrichment of the Inter-Galactic Medium
• Hidden activity in high-redshift spheroidal galaxies from mid-infrared and X-ray observations in the GOODS-North field
• Local and large-scale effects on the astrophysics of void-galaxies
• Silicate-break galaxies: an efficient selection method of distant ultraluminous infrared galaxies
• The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
• The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV & [OII]λ3727 luminosities
• On the Stellar Populations in Faint Red Galaxies in the Hubble Ultra Deep Field
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• VLT/X-Shooter Near-Infrared Spectroscopy and HST Imaging of Gravitationally-Lensed z~2 Compact Quiescent Galaxies
• Cosmic Star Formation: Constraints on the Galaxy Formation Models
• Active Galaxy Nuclei at high redshifts: properties and environment of Type 1 and 2 AGNs
• The age of extremely red and massive galaxies at very high redshift
• Dust-obscured star formation and the contribution of galaxies escaping UV/optical color selections at z~2
• Finite Resolution Deconvolution of Multi-Wavelength Imaging of 20,000 Galaxies in the COSMOS Field: The Evolution of Clumpy Galaxies Over Cosmic Time
• Observations of the High Redshift Universe
• Evolution of the Dependence of Rest-frame Color and Morphology Distribution on Stellar Mass for Galaxies in the Hubble Deep Field North
• The Search for HI Emission at z $\approx 0.4$ in Gravitationally Lensed Galaxies with the Green Bank Telescope
• Holographic Dark Information Energy
• Mass-dependent Color Evolution of Field Galaxies Back to z~3 Over the Wide Range of Stellar Mass
• Are z>2 Herschel galaxies proto-spheroids?
• The Role of Bulge Formation in the Homogenization of Stellar Populations at $z\sim 2$ as revealed by Internal Color Dispersion in CANDELS
• On the discovery of the first 350 micron-selected galaxy
• Lyman Break Galaxies and Reionization of the Universe
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Universe opacity and EBL
• Hydrodynamical Simulations of Galaxy Clusters with Galcons
• Quark-Novae in Neutron Star-White-Dwarf Binaries: A model for luminous (spin-down powered) sub-Chandrasekhar-mass Type Ia Supernovae ?
• The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ) I: IRAC mosaics
• Metal-rich absorbers at high redshifts: abundance patterns
• Selection and Mid-infrared Spectroscopy of Ultraluminous Star-Forming Galaxies at z~2
• Nearby Galaxies in More Distant Contexts
• Understanding galaxy formation with ISO deep surveys
• Spitzer Observations of Red Galaxies: Implication for High-Redshift Star Formation
• An investigation of the star-forming main sequence considering the nebular continuum emission at low-z
• Quantitative interpretation of the rotation curves of spiral galaxies at redshifts z~0.7 and z~1
• Holographic dark information energy: Predicted dark energy measurement
• Dynamics of Lyman Break Galaxies and Their Host Halos
• Detecting Massive Galaxies at High Redshift using the Dark Energy Survey
• The Galaxy Structure-Redshift Relationship
• Faint 6.7um Galaxies and their Contributions to the Stellar Mass Density in the Universe
• A Massive Molecular Gas Reservoir in the z=2.221 Type-2 Quasar Host Galaxy SMM J0939+8315 Lensed by the Radio Galaxy 3C220.3
• The Multi-wavelength Extreme Starburst Sample of Luminous Galaxies Part I: Sample Characteristics
• The impact of binary stars on the colors of high-redshift galaxies
• A Dynamic Dark Information Energy Consistent with Planck Data
• Galaxy Interactions, Star Formation History, and Bulgeless Galaxies
• Low-ionization galaxies and evolution in a pilot survey up to z = 1
• The Star Formation History of Redshift z~2 Galaxies: The Role of The Infrared Prior
• A Submillimeter Continuum Survey of Local Dust-Obscured Galaxies
• Outflows from starburst galaxies with various driving mechanisms and their X-ray properties
• J-PAS: Discovery of RaJav, a bright spatially extended Ly$\alpha$ Nebula at z=2.25
• A Search for Molecular Gas toward a BzK-selected Star-forming Galaxy at z = 2.044
• The Evolution of the Hubble Sequence: morpho-kinematics of distant galaxies
• Massive galaxies at redshift 2 in cosmological hydrodynamic simulations
• What fraction of stars formed in infrared galaxies at high redshift?
• A recent rebuilding of most spirals ?
• The BLOBs: Enigmatic Diffuse Ionized Gas Structures in a Cluster of Galaxies near Cosmic Noon
• Intrinsic colors and ages of extremely red elliptical galaxies at high redshift
• Beyond LCDM: Bits join the Dark Side
• Challenges in Stellar Population Studies
• The Star Formation History and Stellar Assembly of High Redshift Galaxies
• From z>6 to z~2: Unearthing Galaxies at the Edge of the Dark Ages
• 58 Radio Sources Near Bright Natural Guide Stars
• The Accelerating Universe and the Second Law