Audrey Galametz, Daniel Stern, Carlos De Breuck, Nina Hatch, Jack Mayo, George Miley, Alessandro Rettura, Nick Seymour, S. Adam Stanford, Joel Vernet
Taking advantage of the impressive sensitivity of Spitzer to detect massive
galaxies at high redshift, we study the mid-infrared environments of powerful,
high-redshift radio galaxies at 1.2-0.1 (AB), in the fields of 48 radio galaxies at 1.21.2.
Using a counts-in-cell analysis, we identify a field as overdense when 15 or
more red IRAC sources are found within 1arcmin (i.e.,~0.5Mpc at 1.21.2.
View original:
http://arxiv.org/abs/1202.4489
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