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Illuminating the dark side of cosmic star formation two billion years after the Big Bang
Margherita Talia, Andrea Cimatti, Marika Giulietti +5
How and when did galaxies form and assemble their stars and stellar mass? The answer to these questions, so crucial to astrophysics and cosmology, requires the full reconstruction…
The infrared-radio correlation of star-forming galaxies is strongly M-dependent but nearly redshift-invariant since z4
I. Delvecchio, E. Daddi, M. T. Sargent +25
Several works in the past decade have used the ratio between total (rest 8-1000m) infrared and radio (rest 1.4~GHz) luminosity in star-forming galaxies (q), often referre…
A Multi-wavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population
H. S. B. Algera, D. Van der Vlugt, J. A. Hodge +7
Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clear understanding of the relative contribution from radio AGN to be used to their…
An Ultra-deep Multi-band VLA Survey of the Faint Radio Sky (COSMOS-XS): Source Catalog and Number Counts
D. Van der Vlugt, H. S. B. Algera, J. A. Hodge +6
We present ultra-deep, matched-resolution Karl G. Jansky Very Large Array (VLA) observations at 10 and GHz in the COSMOS field: the COSMOS-XS survey. The final 10 and GHz i…
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…