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25 April 2024
 
  » arxiv » astro-ph/0509308

 Article overview



Clustering of Star-forming Galaxies Near a Radio Galaxy at z=5.2
Roderik A. Overzier ; G.K. Miley ; R.J. Bouwens ; N.J.G. Cross ; A.W. Zirm ; N. Benitez ; J.P. Blakeslee ; M. Clampin ; R. Demarco ; H.C. Ford ; G.F. Hartig ; G.D. Illingworth ; A.R. Martel ; H.J.A. Rottgering ; B. Venemans ; the ACS IDT ;
Date 12 Sep 2005
Subject astro-ph
AbstractWe present HST/ACS observations of the most distant radio galaxy known, TN J0924-2201 at z=5.2. This radio galaxy has 6 spectroscopically confirmed Lya emitting companion galaxies, and appears to lie within an overdense region. The radio galaxy is marginally resolved in i_775 and z_850 showing continuum emission aligned with the radio axis, similar to what is observed for lower redshift radio galaxies. Both the half-light radius and the UV star formation rate are comparable to the typical values found for Lyman break galaxies at z~4-5. The Lya emitters are sub-L* galaxies, with deduced star formation rates of 1-10 Msun/yr. One of the Lya emitters is only detected in Lya. Based on the star formation rate of ~3 Msun/yr calculated from Lya, the lack of continuum emission could be explained if the galaxy is younger than ~2 Myr and is producing its first stars. Observations in V_606, i_775, and z_850 were used to identify additional Lyman break galaxies associated with this structure. In addition to the radio galaxy, there are 22 V-break (z~5) galaxies with z_850<26.5 (5sigma), two of which are also in the spectroscopic sample. We compare the surface density of 2/arcmin^2 to that of similarly selected V-dropouts extracted from GOODS and the UDF Parallel fields. We find evidence for an overdensity to very high confidence (>99%), based on a counts-in-cells analysis applied to the control field. The excess is suggestive of the V-break objects being associated with a forming cluster around the radio galaxy.
Source arXiv, astro-ph/0509308
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