Evolution of the red sequence giant to dwarf ratio in galaxy clusters out toz∼ 0.5-Reference-Cited by-同舟云学术

Evolution of the red sequence giant to dwarf ratio in galaxy clusters out toz∼ 0.5

Author:

Bildfell C.¹,Hoekstra H.²,Babul A.¹,Sand D.³,Graham M.³,Willis J.¹,Urquhart S.¹,Mahdavi A.⁴,Pritchet C.¹,Zaritsky D.⁵,Franse J.²,Langelaan P.²

Affiliation:

1. Department of Physics & Astronomy; University of Victoria; Victoria; BC; V8P 1A1; Canada

2. Leiden Observatory; Leiden University; PO Box 9513; NL-2300 RA Leiden; the Netherlands

3. Las Cumbres Observatory Global Telescope Network; 6740 Cartona Drive, Suite 102; Santa Barbara; CA; 93117; USA

4. Department of Physics & Astronomy; San Francisco State University; San Francisco; CA; 94131; USA

5. Steward Observatory; University of Arizona; Tucson; AZ; 85721; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference52 articles.

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