Abstract
From examination of only 4 deg2 of sky in the NOAO Deep Wide-Field Survey (NDWFS) region, we have identified the first radio-loud quasar at a redshift z > 6. The object, FIRST J1427385+331241, was discovered by matching the FLAMINGOS Extragalactic Survey (FLAMEX) IR survey to Faint Images of the Radio Sky at Twenty cm (FIRST) survey radio sources with NDWFS counterparts. One candidate z > 6 quasar was found, and spectroscopy with the Keck II telescope confirmed its identification yielding a redshift z = 6.12. The object is a broad absorption line (BAL) quasar with an optical luminosity of MB ~ -26.9 and a radio-to-optical flux ratio ~60. Two Mg II absorptions systems are present at redshifts of z = 2.18 and z = 2.20. We briefly discuss the implications of this discovery for the high-redshift quasar population.
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CITATION STYLE
McGreer, I. D., Becker, R. H., Helfand, D. J., & White, R. L. (2006). Discovery of a z = 6.1 Radio‐Loud Quasar in the NOAO Deep Wide Field Survey. The Astrophysical Journal, 652(1), 157–162. https://doi.org/10.1086/507767
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