Extragalactic radio surveys in the pre-Square Kilometre Array era
arXiv:1706.06603
Abstract
The era of the Square Kilometre Array is almost upon us, and pathfinder telescopes are already in operation. This brief review summarizes our current knowledge of extragalactic radio sources, accumulated through six decades of continuum surveys at the low-frequency end of the electromagnetic spectrum and the extensive complementary observations at other wavelengths necessary to gain this understanding. The relationships between radio survey data and surveys at other wavelengths are discussed. Some of the outstanding questions are identified and prospects over the next few years are outlined.
arXiv commentInvited review for Royal Society Open Science, 22 pages
References in corpus (50)
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- On the normalisation of the cosmic star formation history
- The host galaxies of radio-loud AGN: mass dependencies, gas cooling and AGN feedback
- Radio-Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications
- Distant Radio Galaxies and their Environments
- A median redshift of 2.4 for galaxies bright at submillimetre wavelengths
- The VISTA Deep Extragalactic Observations (VIDEO) Survey
- A semi-empirical simulation of the extragalactic radio continuum sky for next generation radio telescopes
- The Nature and Evolution of Classical Double Radio Sources from Complete Samples
- Mapping the Evolution of High Redshift Dusty Galaxies with Submillimeter Observations of a Radio-Selected Sample
- The radio luminosity function from the low-frequency 3CRR, 6CE & 7CRS complete samples
- Radio and Millimeter Continuum Surveys and their Astrophysical Implications
- The Radio-to-Submm Spectral Index as a Redshift Indicator
- Near-infrared imaging and the K-z relation for radio galaxies in the 7C Redshift Survey
- Radio Emission from Galaxies In The Hubble Deep Field
- The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population
- The obscuration by dust of most of the growth of supermassive black holes
- The Connection Between Radio Quiet AGN and the High/Soft State of X-Ray Binaries
- The Phoenix Deep Survey: The 1.4 GHz microJansky catalogue
- Radio Continuum Imaging of High Redshift Radio Galaxies
- The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5
- The relationship between radio luminosity and black-hole mass in optically-selected quasars
- A new method to separate star forming from AGN galaxies at intermediate redshift: The submillijansky radio population in the VLA-COSMOS survey
- The Nature of Radio-Intermediate Quasars: What is Radio-Loud and what is Radio-Quiet?
- Deep multi-frequency radio imaging in the Lockman Hole using the GMRT and VLA: I. The nature of the sub-mJy radio population
- AGN and Starburst Radio Emission from Optically Selected QSOs
- Star formation in quasar hosts and the origin of radio emission in radio-quiet quasars
- The cosmic evolution of radio-AGN feedback to z=1
- Radio imaging of the Subaru/XMM-Newton Deep Field - III. Evolution of the radio luminosity function beyond z=1
- The Two-Component Radio Luminosity Function of QSOs: Star Formation and AGN
- The central engines of radio-quiet quasars
- A Deep VLA survey at 20cm of the ISO ELAIS survey regions
- GAMA/WiggleZ: The 1.4GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z=0.75
- Clustering of Star-forming Galaxies Near a Radio Galaxy at z=5.2
- The luminosity-dependent high-redshift turnover in the steep spectrum radio luminosity function: clear evidence for downsizing in the radio-AGN population
- The nature of the bright submillimeter galaxy population: a radio pre-selected sample with I>25
- A sample of 6C radio sources with virtually complete redshifts. II - optical spectroscopy
- A Combined EIS-NVSS Survey Of Radio Sources (CENSORS) III: Spectroscopic observations
- Observational constraints on the spin of the most massive black holes from radio observations
- The cosmic evolution of low-luminosity radio sources from the SDSS DR1
- Sample variance, source clustering and their influence on the counts of faint radio sources
- The Likelihood Ratio as a tool for Radio Continuum Surveys with SKA precursor telescopes
- Unveiling the origin of the radio emission in radio-quiet quasars
- The discovery of a typical radio galaxy at z = 4.88
- The radio properties of infrared-faint radio sources
- The hyperluminous infrared quasar 3C 318 and its implications for interpreting sub-mm detections of high-redshift radio galaxies
- Black hole spin and size of the X-ray emitting region(s) in the Seyfert 1.5 galaxy ESO 362-G18
- The hard X-ray spectrum of NGC 1365: scattered light, not black hole spin
- A new search for distant radio galaxies in the Southern hemisphere -- II. 2.2 micron imaging
- The Spin of the Supermassive Black Hole in MCG-05-23-16