The spatial clustering of ultraluminous infrared galaxies over 1.5<z<3

Details The spatial clustering of ultraluminous infrared galaxies over 1.5<z<3 The spatial clustering of ultraluminous infrared galaxies over 1.5<z<3

2006-03-02

arxiv.org/abs/astro-ph/0603061v2

Erratum-ibid.643:L139,2006; Astrophys.J.641:L17-L20,2006

Astronomy and Astrophysics

Astrophysics

ApJ Letters, accepted. Updated to correct an error in the correlation length calculations

Scientific paper

10.1086/505266

We present measurements of the spatial clustering of galaxies with stellar masses >10^11Msun, infrared luminosities >10^12 Lsun, and star formation rates >200Msun per year in two redshift intervals; 1.51, both starbursts and AGN. Adopting plausible models for the growth of DM haloes with redshift, then the haloes hosting the 21 signpost stellar buildup in galaxies that will reside in clusters at z=0, with ULIRGs at increasing redshifts signposting the buildup of stars in galaxies that will reside in increasingly rich clusters.

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