Faint submillimeter galaxies identified through their optical/near-infrared colors: 1. Spatial clustering and halo masses

Faint submillimeter galaxies identified through their optical/near-infrared colors: 1. Spatial clustering and halo masses

The properties of submillimeter galaxies (SMGs) that are fainter than the confusion limit of blank-field single-dish surveys (S850  2 mJy) are poorly constrained. Using a newly developed color selection technique, Optical-Infrared Triple Color (OIRTC), that has been shown to successfully select suc...

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Bibliographic Details
Main Authors: Chen (陳建州), Chian-Chou, Smail, Ian, Swinbank, A.M., Simpson, James M., Almaini, Omar, Conselice, Christopher J., Hartley, Will G., Mortlock, Alice, Simpson, Chris, Wilkinson, Aaron
Format: Article
Published: American Astronomical Society 2016
Subjects:
cosmology: observations ; galaxies: evolution ; galaxies: formation ; galaxies: high-redshift ; largescale structure of universe ; submillimeter: galaxies
Online Access:https://eprints.nottingham.ac.uk/39817/

Internet

https://eprints.nottingham.ac.uk/39817/

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