S.C. Chapman
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
A. Blain
R. Ibata
R.J. Ivison
Professor 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 |
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