Fig. 4 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. 4.

Plot of the log P_{1.4 GHz} against log L_FIR showing our new FF sample as solid triangles, along with several comparison samples taken from the literature. Three well‐known ULIGs are marked by name. Radio‐loud quasars and BL Lacs are included at the most luminous end of the track traced by the Texas‐FSC sources. The luminosities for F10214 have been corrected for gravitational lensing.

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