The FIR-Radio Relationship at High and Low Redshift

Abstract

We use the results of the SCUBA Local Universe Galaxy Survey, a submillimetre survey of galaxies in the nearby Universe, to investigate the relationship between the far-infrared--submillimetre and radio emission of galaxies at both low and high redshift. At low redshift we show that the correlation between radio and far-infrared emission is much stronger than the correlation between radio and submillimetre emission, which is evidence that massive stars are the source of both the far-infrared and radio emission. At high redshift we show that the submillimetre sources detected by SCUBA are brighter sources of radio emission than are predicted from the properties of galaxies in the local Universe. We discuss possible reasons for the cosmic evolution of the relationship between radio and far-infrared emission.

arXiv comment8 pages including 4 figures. Version accepted for publication in MNRAS

References in corpus (24)

• Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
• A Deep Sub-millimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution
• A Redshift Survey of the Submillimeter Galaxy Population
• Radio Properties of Infrared Selected Galaxies in the IRAS 2 Jy Sample
• The SCUBA Local Universe Galaxy Survey I: First Measurements of the Submillimetre Luminosity and Dust Mass Functions
• The Canada-UK Deep Submillimetre Survey: First Submillimetre Images, the Source Counts, and Resolution of the Background
• The SCUBA Local Universe Galaxy Survey II. 450 micron data - evidence for cold dust in bright IRAS Galaxies
• SHARC-2 350 Micron Observations of Distant Submillimeter Selected Galaxies
• The Far- and Mid-Infrared/Radio Correlations in the Spitzer Extragalactic First Look Survey
• Magnetic Fields in Starburst Galaxies and The Origin of the FIR-Radio Correlation
• Evidence for extended, obscured starbursts in submm galaxies
• Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: I. The role of ISM pressure & the Molecular Cloud Dissipation Timescale
• The Scatter in the Relationship between Redshift and the Radio-to-Submm Spectral Index
• The FIR/Radio correlation of high redshift galaxies in the HDF-N
• The SCUBA Local Universe Galaxy Survey - III. Dust along the Hubble sequence
• The optical-to-radio spectral energy distributions of low-metallicity blue compact dwarf galaxies
• An Initial Look at the Far Infrared-Radio Correlation within Nearby Star-forming Galaxies using the Spitzer Space Telescope
• Dust temperture and the submillimetre-radio flux density ratio as a redshift indicator for distant galaxies
• Constraining the Radio-Submm Redshift Indicator using data from the SCUBA Local Universe Galaxy Survey
• The Molecular Connection to the FIR-Radio Continuum Correlation in Galaxies
• XMM-Newton Surveys of the CFRS Fields - I: The Sub-mm/X-ray relation
• The Radio-FIR correlation: Is MHD Turbulence the Cause?
• The far-IR/radio correlation in the ISO era
• Modeling the evolution of infrared luminous galaxies: the influence of the Luminosity-Temperature distribution

Cited by in corpus (36)

• Determining Star Formation Rates for Infrared Galaxies
• An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies
• Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly
• The Physics of the FIR-Radio Correlation: I. Calorimetry, Conspiracy, and Implications
• The Herschel Reference Survey: Dust in Early-Type Galaxies and Across the Hubble Sequence
• The Star Formation History of the Universe as Revealed by Deep Radio Observations
• Rapid dust production in submillimeter galaxies at z>4?
• GOODS-Herschel: radio-excess signature of hidden AGN activity in distant star-forming galaxies
• An Accounting of the Dust-Obscured Star Formation and Accretion Histories Over the Last ~11~Billion Years
• Planck's Dusty GEMS: Gravitationally lensed high-redshift galaxies discovered with the Planck survey
• The Properties of Sub-mm Galaxies in Hierarchical Models
• The VLA-COSMOS Perspective on the IR-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the IR/Radio Properties of Star Forming and AGN Galaxies at Intermediate and High Redshift
• The Physics of the FIR-Radio Correlation: II. Synchrotron Emission as a Star-Formation Tracer in High-Redshift Galaxies
• Herschel-ATLAS: The far-infrared--radio correlation at z<0.5
• Mid-Infrared Spectroscopy of Lensed Galaxies at 1<z<3: The Nature of Sources Near the MIPS Confusion Limit
• The nature of GRB-selected submillimeter galaxies: hot and young
• Evolution of the Far-Infrared-Radio Correlation and Infrared SEDs of Massive Galaxies over z = 0 - 2
• Sources of the Radio Background Considered
• A closer view of the radio-FIR correlation: disentangling the contributions of star formation and AGN activity
• Ultradeep Near-Infrared Observations of GOODS 850-5
• The Star-Forming Galaxy Contribution to the Cosmic MeV and GeV Gamma-Ray Background
• The temperature dependence of the far-infrared-radio correlation in the Herschel-ATLAS
• CHANG-ES VI: Probing Supernova Energy Deposition in Spiral Galaxies Through Multi-Wavelength Relationships
• A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2
• A 610-MHz survey of the Lockman Hole with the Giant Metrewave Radio Telescope - I. Observations, data reduction and source catalogue for the central 5 square degrees
• AEGIS: Radio and Mid-Infrared Selection of Obscured AGN Candidates
• Discovery of Peculiar Radio Morphologies with ASKAP using Unsupervised Machine Learning
• Kinematic signatures of AGN feedback in moderately powerful radio galaxies at z~2 observed with SINFONI
• The contribution of star-forming galaxies to the cosmic radio background
• Multi-wavelength lens reconstruction of a $\text{Planck}$ $\&$ $\text{Herschel}$-detected star-bursting galaxy
• On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths
• Central free-free-dominated 880 $\micron$ emission in II Zw 40
• The Cold Dust Content of the Nearby Galaxies IC 5325, NGC 7496, NGC 7590, and NGC 7599
• CO investigation of z=0.4-1.5 galaxies
• Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
• Dust content of core-collapse supernova hosts