A large Hα survey at z=2.23, 1.47, 0.84 & 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS
arXiv:1202.3436 · doi:10.1093/mnras/sts096
Abstract
This paper presents new deep and wide narrow-band surveys undertaken with UKIRT, Subaru and the VLT; a combined effort to select large, robust samples of H-alpha (Ha) emitters at z=0.40, 0.84, 1.47 and 2.23 (corresponding to look-back times of 4.2, 7.0, 9.2 and 10.6 Gyrs) in a uniform manner over ~2 deg^2 in the COSMOS and UDS fields. The deep Ha surveys reach ~3M_sun/yr out to z=2.2 for the first time, while the wide area and the coverage over two independent fields allow to greatly overcome cosmic variance. A total of 1742, 637, 515 and 807 Ha emitters are homogeneously selected at z=0.40, 0.84, 1.47 and 2.23, respectively, and used to determine the Ha luminosity function and its evolution. The faint-end slope is found to be -1.60+-0.08 over z=0-2.23, showing no evolution. The characteristic luminosity of SF galaxies, L*, evolves significantly as log[L*(z)]=0.45z+log[L*(z=0)]. This is the first time Ha has been used to trace SF activity with a single homogeneous survey at z=0.4-2.23. Overall, the evolution seen in Ha is in good agreement with the evolution seen using inhomogeneous compilations of other tracers of star formation, such as FIR and UV, jointly pointing towards the bulk of the evolution in the last 11 Gyrs being driven by a strong luminosity increase from z~0 to z~2.2. Our uniform analysis reveals an Ha star formation history of the Universe which can be simply parameterised by log(SFRD)=-2.1/(1+z) for z<2.23. Both the shape and normalisation of the Ha star formation history are consistent with the measurements of the stellar mass density growth, confirming that our Ha analysis traces the bulk of the formation of stars in the Universe up to z~2.2. Star formation activity since z~2.2 is responsible for ~95% of the total stellar mass density observed locally today (with half being assembled between z=1.2-2.2, and the rest since z<1.2).
20 pages, 11 Figures, accepted for publication in MNRAS. Sample of z=2.23 emitters increased to 807 after completing the COSMOS survey
References in corpus (20)
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- The Cosmic Evolution Survey (COSMOS) -- Overview
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
- The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN
- Subaru Deep Survey V. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Photometric Properties
- The Gemini Deep Deep Survey: III. The abundance of massive galaxies 3-6 billion years after the Big Bang
- Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source population
- The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for Narrow-band Emitters in the Subaru Deep Field
- HiZELS: a high redshift survey of H-alpha emitters. I: the cosmic star-formation rate and clustering at z=2.23
- The Evolution of the UV Luminosity Function from z ~ 0.75 to z ~ 2.5 using HST ERS WFC3/UVIS Observations
- The H-alpha Luminosity Function and Star Formation Rate Volume Density at z=0.8 from the NEWFIRM H-alpha Survey
- The clustering of H-alpha emitters at z=2.23 from HiZELS
- The Halpha-based Star Formation Rate Density of the Universe at z=0.84
- The H Luminosity Function and Star Formation Rate at in the Cosmos 2 Square-Degree Field
- The impact of Spitzer infrared data on stellar mass estimates - and a revised galaxy stellar mass function at 0 < z < 5
- A Pilot Survey for KX QSOs in the UKIDSS Ultra Deep Survey Field
- The Evolution of the Rest-frame V-band Luminosity Function from z=4: A Constant Faint-end Slope over the Last 12 Gyr of Cosmic History
- Spectroscopic follow-up of a cluster candidate at z = 1.45
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- Holographic dark information energy: Predicted dark energy measurement
- The OTELO survey: the star formation rate evolution of low-mass galaxies
- A comprehensive study of H emitters at 0.62 in the DAWN survey: the need for deep and wide regions
- Kinematic Lensing with the Roman Space Telescope
- Multiple emission lines of H emitters at from the broad and medium-band photometry in the ZFOURGE Survey
- Euclid preparation. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
- Subaru/HSC z-Broadband Excess Selection of Extreme Emission Line Galaxies at z<1
- Properties of galaxies at the faint end of the H luminosity function at
- The H luminosity and stellar mass dependent clustering of star-forming galaxies at with 3D-HST
- A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)
- The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
- Non-Gaussian assembly bias from a semi-analytic galaxy formation model
- HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
- The nature of [S III]λλ9096, 9532 emitters at z = 1.34 and 1.23
- Universal conditional distribution function of [OII] luminosity of galaxies, and prediction for the [OII] luminosity function at redshift
- Evolution of the cold gas fraction and the star formation history: Prospects with current and future radio facilities
- Modeling spatially-resolved galactic H emission for galaxy clustering
- Emission Line Galaxies in the SHARDS Hubble Frontier Fields II: Limits on Lyman-Continuum Escape Fractions of Lensed Emission Line Galaxies at Redshifts 2 < z < 3.5
- Evidence of Increased UV FeII Emission in Quasars in Candidate Overdense Regions
- The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
- Phenomenological power spectrum models for H emission line galaxies from the Nancy Grace Roman Space Telescope
- Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
- Quantifying the effect of field variance on the H luminosity function with the New Numerical Galaxy Catalogue (GC)
- Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
- The Properties of the Star-Forming Interstellar Medium at z=0.84-2.23 from HiZELS - I: Mapping the Internal Dynamics and Metallicity Gradients in High-Redshift Disk Galaxies
- The Properties of the Star-Forming Interstellar Medium at z=0.8-2.2 from HiZELS - II: Star-Formation and Clump Scaling Laws in Gas Rich, Turbulent Disks
- Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope
- The Physical Properties of Star-Forming Galaxies with Strong [O III] Lines at z=3.25
- Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
- Extended H over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at
- Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
- COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 m Since