57 citations · 80 across the 3 of their papers we have counts for
6 papers
The non-linear infrared-radio correlation of low-z galaxies: implications for redshift evolution, a new radio SFR recipe, and how to minimize selection bias
Daniel Cs. Molnar, Mark T. Sargent, Sarah Leslie +7
The infrared-radio correlation (IRRC) underpins many commonly used radio luminosity-star formation rate (SFR) calibrations. In preparation for the new generation of radio surveys w…
FR-type radio sources at 3 GHz VLA-COSMOS: Relation to physical properties and large-scale environment
E. Vardoulaki, E. F. Jiménez Andrade, I. Delvecchio +16
() We probe the physical properties and large-scale environment of radio AGN in the faintest FR population to-date, and link them to their radio structure. We use the VLA…
The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of active galactic nuclei
Krešimir Tisanić, V. Smolčić, M. Imbrišak +5
As the SKA is expected to be operational in the next decade, investigations of the radio sky in the range of 100 MHz to 10 GHz have become important for simulations of the SKA obse…
The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT continuum observations
B. Slaus, V. Smolcic, M. Novak +15
We study the space density evolution of active galactic nuclei (AGN) using the radio survey of the XXL-North field, performed with the Giant Metrewave Radio Te…
A closer look at the deep radio sky: Multi-component radio sources at 3-GHz VLA-COSMOS
E. Vardoulaki, E. F. Jiménez Andrade, A. Karim +20
In this data paper we present and characterise the multi-component radio sources identified in the VLA-COSMOS Large Project at 3 GHz (0.75 arcsec resolution, 2.3 μJy/beam rms), i.e…
The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of highly star-forming galaxies
K. Tisanić, V. Smolčić, J. Delhaize +7
We construct the average radio spectral energy distribution (SED) of highly star-forming galaxies (HSFGs) up to z~4. Infrared and radio luminosities are bound by a tight correlatio…