Fig. 1 from The FIRST Sample of Ultraluminous Infrared Galaxies at High Redshift. I. Sample and Near‐Infrared Morphologies

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The FIRST Sample of Ultraluminous Infrared Galaxies at High Redshift. I. Sample and Near‐Infrared Morphologies

Authors: S. A. Stanford, Daniel Stern, Wil van Breugel, and Carlos De Breuck

Stanford, Stern, van Breugel, & De Breuck 2000 The Astrophysical Journal Supplement Series 131 185.

Provider: AAS Journals

Caption: Fig. 1.

Plot of F_ν at 1.4 GHz against F_ν at 60 μm showing all matches of the positional cross‐correlation of FIRST with the IRAS FSC (solid triangles), along with several comparison samples taken from the literature. The well‐known radio–FIR correlation for star‐forming galaxies extends to the faintest flux limits probed by the FF objects.

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