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
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 |
You might also like
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search