Open AccessThe environments of hyperluminous infrared galaxies at 0.44 < z < 1.55
Author(s) -
Farrah D.,
Geach J.,
Fox M.,
Serjeant S.,
Oliver S.,
Verma A.,
Kaviani A.,
RowanRobinson M.
Publication year - 2004
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2004.07515.x
Subject(s) - physics , astrophysics , qsos , luminous infrared galaxy , galaxy , astronomy , galaxy merger , redshift , lenticular galaxy , galaxy formation and evolution , galaxy group , interacting galaxy
We present deep wide‐field K s ‐band observations of six Hyperluminous Infrared Galaxies (HLIRGs) spanning a redshift range 0.44 < z < 1.55 . The sample resides in a wide variety of environments, from the field to Abell 2 clusters, with a mean galaxy–HLIRG clustering amplitude of 〈 B gh 〉= 190 ± 45 Mpc 1.77 . The range in environments, and the mean clustering level, are both greater than those seen in local IR‐luminous galaxies, from which we infer that the range of galaxy evolution processes driving IR‐luminous galaxy evolution at z > 0.5 is greater than locally, and includes mergers between gas‐rich spiral galaxies in the field, but also includes encounters in clusters and hierarchical build‐up. The similarity in the range of environments and mean clustering amplitude between our sample and QSOs over a similar redshift range is consistent with the interpretation where evolutionary connections between IR‐luminous galaxies and QSOs are stronger at z > 0.5 than locally, and that, at these redshifts, the processes that drive QSO evolution are similar to those that drive IR‐luminous galaxy evolution. From comparison of the HLIRG and QSO host galaxies we further postulate that a larger fraction of IR‐luminous galaxies pass through an optical QSO stage at z > 0.5 than locally.