The conditional colour–magnitude distribution – I. A comprehensive model of the colour–magnitude–halo mass distribution of present-day galaxies

Journal Article · 25 September 2018 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/sty2615 · OSTI ID:1477805

Xu, Haojie  ^[1]; Zheng, Zheng ^[2]; Guo, Hong ^[3]; Zu, Ying  ^[4]; Zehavi, Idit ^[5]; Weinberg, David H. ^[6]

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1. Department of Physics and Astronomy, University of Utah, 115 South 1400 East, Salt Lake City, UT 84112, USA, Department of Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
2. Department of Physics and Astronomy, University of Utah, 115 South 1400 East, Salt Lake City, UT 84112, USA, Department of Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China, Tsung-Dao Lee Institute, Shanghai 200240, China
3. Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Shanghai 200030, China
4. Department of Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China, Department of Astronomy, Ohio State University, Columbus, OH 43210, USA, Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USA
5. Department of Astronomy and Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, OH 44106, USA
6. Department of Astronomy, Ohio State University, Columbus, OH 43210, USA, Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USA

• Sponsoring Organization: USDOE
• OSTI ID: 1477805
• Journal Information: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Vol. 481 Journal Issue: 4; ISSN 0035-8711
• Publisher: Oxford University PressCopyright Statement
• Country of Publication: United Kingdom
• Language: English