NAM logo, by David Le Conte


ELAIS : A deep survey with the ISO satellite

Paolo Ciliegi (Bologna)

A well-know tight, linear correlation is present between the far infrared flux measured by IRAS and the nonthermal radio flux density (at 1.4 GHz) from disk of spiral galaxies. This correlation defines a ratio of infrared to radio fluxes that is characteristic of star formation activity.

We used a deep VLA radio survey (5 sigma limit of 0.135 mJy at 1.4 GHz) in the same region of the sky that have been surveyed over the wavelength range 6.7 - 175 microns with ISO (as part of the European Large Area ISO Survey, ELAIS) to study the radio far-infrared correlation to a flux density deeper than that reached by IRAS. The radio far-infrared correlation is expected to extend below the IRAS flux level since the majority of the sub-mJy radio sources have been identified with the faint blue galaxies with spectra similar to those of star forming objects.


Maintained by Ian Howarth