Galaxy And Mass Assembly: The 1.4GHz SFR indicator, SFR-M* relation and predictions for ASKAP-GAMA
arXiv:1701.06242 · doi:10.1093/mnras/stw3080
Abstract
We present a robust calibration of the 1.4GHz radio continuum star formation rate (SFR) using a combination of the Galaxy And Mass Assembly (GAMA) survey and the Faint Images of the Radio Sky at Twenty-cm (FIRST) survey. We identify individually detected 1.4GHz GAMA-FIRST sources and use a late-type, non-AGN, volume-limited sample from GAMA to produce stellar mass-selected samples. The latter are then combined to produce FIRST-stacked images. This extends the robust parametrisation of the 1.4GHz-SFR relation to faint luminosities. For both the individually detected galaxies and our stacked samples, we compare 1.4GHz luminosity to SFRs derived from GAMA to determine a new 1.4GHz luminosity-to-SFR relation with well constrained slope and normalisation. For the first time, we produce the radio SFR-M* relation over 2 decades in stellar mass, and find that our new calibration is robust, and produces a SFR-M* relation which is consistent with all other GAMA SFR methods. Finally, using our new 1.4GHz luminosity-to-SFR calibration we make predictions for the number of star-forming GAMA sources which are likely to be detected in the upcoming ASKAP surveys, EMU and DINGO.
14 pages, 6 figures
References in corpus (17)
- A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
- Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
- The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
- The VLA-COSMOS Survey: II. Source Catalog of the Large Project
- A Turnover in the Galaxy Main Sequence of Star Formation at for Redshifts
- Signals from the Noise: Image Stacking for Quasars in the FIRST Survey
- The Star Formation History of the Universe as Revealed by Deep Radio Observations
- Spitzer Mid-to-Far-Infrared Flux Densities of Distant Galaxies
- The VLA 1.4GHz Survey of the Extended Chandra Deep Field South: First Data Release
- Radio galaxies in the 2SLAQ Luminous Red Galaxy Survey: I. The evolution of low-power radio galaxies to z~0.7
- The Radio Continuum-Star Formation Rate Relation in WSRT SINGS Galaxies
- Galaxy And Mass Assembly (GAMA): Active Galactic Nuclei in Pairs of Galaxies
- The Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS): Survey design, data catalogue and GAMA/WiggleZ spectroscopy
- ATLAS 1.4 GHz Data Release 2 -- I. Observations of the CDF-S and ELAIS-S1 fields and methods for constructing differential number counts
- Halpha Imaging of the Herschel Reference Survey. The star formation properties of a volume-limited, K-band-selected sample of nearby late-type galaxies
- Emission from Very Small Grains and PAH Molecules in Monte Carlo Radiation Transfer Codes: Application to the Edge-On Disk of Gomez's Hamburger
- Radio--Far infrared correlation in "blue cloud" galaxies with 0<z<1.2
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