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Do Submillimeter Galaxies Really Trace the Most Massive Dark-Matter Halos? Discovery of a High-z Cluster in a Highly Active Phase of Evolution

Chapman, S.C.; Blain, A.; Ibata, R.; Ivison, R.J.; Smail, I.; Morrison, G.

Authors

S.C. Chapman

A. Blain

R. Ibata

R.J. Ivison

Profile image of Ian Smail

Ian Smail ian.smail@durham.ac.uk
Emeritus Professor

G. Morrison



Citation

Chapman, S., Blain, A., Ibata, R., Ivison, R., Smail, I., & Morrison, G. (2009). Do Submillimeter Galaxies Really Trace the Most Massive Dark-Matter Halos? Discovery of a High-z Cluster in a Highly Active Phase of Evolution. Astrophysical Journal, 691, 560-568. https://doi.org/10.1088/0004-637x/691/1/560

Journal Article Type Article
Publication Date 2009-01
Journal \apj
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Volume 691
Pages 560-568
DOI https://doi.org/10.1088/0004-637x/691/1/560
Public URL https://durham-repository.worktribe.com/output/1519463
Publisher URL http://adsabs.harvard.edu/abs/2009ApJ...691..560C