A radio galaxy at z=5.19

被引:134
作者
van Breugel, W [1 ]
De Breuck, C
Stanford, SA
Stern, D
Röttgering, H
Miley, G
机构
[1] Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94550 USA
[2] Leiden Observ, NL-2300 RA Leiden, Netherlands
[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
关键词
early universe; galaxies : active; galaxies : distances and redshifts galaxies : formation; galaxies : individual (TN J0924-2201);
D O I
10.1086/312080
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of the most distant known active galactic nucleus, the radio galaxy TN J0924-2201 at z = 5.19. The radio source was selected from a new sample of ultrasteep spectrum sources, has an extreme radio spectral index alpha(365 MHz)(1.4 GHz) = -1.63, and is identified at near-IR wavelengths with a very faint, K = 21.3 +/- 0.3 object. Spectroscopic observations show a single emission line at lambda similar to 7530 Angstrom, which we identify as Ly alpha. The K-band image, sampling rest-frame U band, shows a multicomponent, radio-aligned morphology, which is typical of lower-redshift radio galaxies. TN J0924-2201 extends the near-IR Hubble, or K-z, relation for powerful radio galaxies to z > 5 and is consistent with models of massive galaxies forming at even higher redshifts.
引用
收藏
页码:L61 / L64
页数:4
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