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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. 3.

For each of the FF objects in Table 1 we show on the left the DSS finding chart centered on the FIRST radio position, which is marked by a small circle of diameter 5﹩\arcsec﹩, with the FSC 95% confidence limit error ellipse superposed. The astrometric uncertainty between the optical and radio reference frames is ~1﹩\arcsec﹩. On the right in each panel is a close‐up view of the K‐band image of the identified source. North is up and east to the left in all panels.

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