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HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements

Publication status:: Published

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APA Style

Cooray, A., Amblard, A., Wang, L., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chanial, P., Clements, D., Conley, A., Conversi, L., Dowell, C., … Franceschini, A. (2010). HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements. ASTRONOMY and ASTROPHYSICS, 518, L22–L22.

MLA Style

Cooray, A, et al. “HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements.” ASTRONOMY and ASTROPHYSICS, vol. 518, 2010, pp. L22–L22.

Chicago Style

Cooray, A, A Amblard, L Wang, et al. 2010. “HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements.” ASTRONOMY and ASTROPHYSICS 518: L22–L22.
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Publisher copy:: 10.1051/0004-6361/201014597

Authors

+ Cooray, A More by this author

Role:: Author

+ Amblard, A More by this author

Role:: Author

+ Wang, L More by this author

Role:: Author

+ Arumugam, V More by this author

Role:: Author

+ Auld, R More by this author

Role:: Author

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Journal:: ASTRONOMY and ASTROPHYSICS More from this journal
Volume:: 518
Pages:: L22-L22
Publication date:: 2010-01-01
DOI:: 10.1051/0004-6361/201014597
EISSN:: 1432-0746
ISSN:: 0004-6361

Language:: English
Keywords:: submillimeter: galaxies

galaxies: evolution

galaxies: high-redshift

large-scale structure of Universe

cosmology: observations
Pubs id:: pubs:93233
UUID:: uuid:05e8bf6b-909c-466f-98f3-b244b5f51c56
Local pid:: pubs:93233
Source identifiers:: 93233
Deposit date:: 2012-12-19
ARK identifier:: ark:/29072/ora_05e8bf6b909c466f98f3b244b5f51c56

Terms of use

Copyright date:: 2010

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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