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

Duncan Farrah·Carol Lonsdale·Colin Borys·Fan Fang·Ian Waddington·Seb Oliver·Michael Rowan-Robinson·Tom Babbedge·David Shupe·Mari Polletta·Harding Smith·Jason Surace
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Abstract

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; 1.5 1, both starbursts and AGN. Adopting plausible models for the growth of DM haloes with redshift, then the haloes hosting the 2 1 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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Duncan Farrah, Carol Lonsdale, Colin Borys, Fan Fang, Ian Waddington, Seb Oliver, Michael Rowan-Robinson, Tom Babbedge, David Shupe, Mari Polletta, Harding Smith, Jason Surace. 2006-04-20. The spatial clustering of ultraluminous infrared galaxies over 1.5<z<3. https://doi.org/10.1086/505266

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