Evolution of the red sequence giant to dwarf ratio in galaxy clusters out to z ∼ 0.5
Version of Record online: 30 JUL 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 425, Issue 1, pages 204–221, 1 September 2012
How to Cite
Bildfell, C., Hoekstra, H., Babul, A., Sand, D., Graham, M., Willis, J., Urquhart, S., Mahdavi, A., Pritchet, C., Zaritsky, D., Franse, J. and Langelaan, P. (2012), Evolution of the red sequence giant to dwarf ratio in galaxy clusters out to z ∼ 0.5. Monthly Notices of the Royal Astronomical Society, 425: 204–221. doi: 10.1111/j.1365-2966.2012.21426.x
- Issue online: 20 AUG 2012
- Version of Record online: 30 JUL 2012
- Manuscript Accepted: 30 MAY 2012
- Manuscript Received: 9 MAY 2012
- Marie Curie International Reintegration. Grant Number: 230924
- Netherlands Organization for Scientific Research. Grant Number: 639.042.814
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