Infrared-radio relation in the local Universe

  title={Infrared-radio relation in the local Universe},
  author={K. Tisani'c and Gianfranco de Zotti and Amirnezam Amiri and Anita Khoram and Saeed Tavasoli and Z. Vidovi'c-Tisani'c},
  journal={Astronomy \& Astrophysics},
Context. The Square Kilometer Array (SKA) is expected to detect high-redshift galaxies with star formation rates (SFRs) up to two orders of magnitude lower than Herschel surveys and will thus boost the ability of radio astronomy to study extragalactic sources. The tight infrared-radio correlation offers the possibility of using radio emission as a dust-unobscured star formation diagnostic. However, the physics governing the link between radio emission and star formation is poorly understood… 

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Astronomy and Astrophysics (ISSN 0004-6361)
  • Astronomical Society,
  • 1989
Cosmic Star Formation History Measured at 1.4 GHz
We matched the 1.4 GHz local luminosity functions of star-forming galaxies (SFGs) and active galactic nuclei to the 1.4 GHz differential source counts from 0.25 μJy to 25 Jy using combinations of
Advancing Astrophysics with the Square Kilometre Array
Astronomical Data Analysis
The infrared-radio relation in the local universe