Spitzer Observations of Deep VLA Fields: Assessing the Total Infrared Luminosity Estimates for z ⪆ 1 Galaxies

Details Spitzer Observations of Deep VLA Fields: Assessing the Total Infrared Luminosity Estimates for z ⪆ 1 Galaxies Spitzer Observations of Deep VLA Fields: Assessing the Total Infrared Luminosity Estimates for z ⪆ 1 Galaxies

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..399..182e&link_type=abstract

Panoramic Views of Galaxy Formation and Evolution ASP Conference Series, Vol. 399, proceedings of the conference held 11-16 Dece

Astronomy and Astrophysics

Astronomy

Scientific paper

Because of the tight correlation between the radio and infrared luminosities known to hold among star-forming galaxies, deep VLA 1.4 GHz data are expected to provide accurate and robust estimates for the total infrared luminosities of the star-forming component in high-redshift galaxies. Here, we compare the radio-derived total infrared luminosities with those derived from the Spitzer/MIPS 24 μm observations, examining the consistency/discrepancy of these two types of estimates.

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