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How sensitive are predicted galaxy luminosities to the choice of stellar population synthesis model?
V. Gonzalez-Perez, C. G. Lacey, C. M. Baugh, et al. Monthly Notices of the Royal Astronomical Society 439(1) 264 (2014) https://doi.org/10.1093/mnras/stt2410
Massive, red galaxies in a hierarchical universe - II. Clustering of Extremely Red Objects
Number Density Evolution ofKs‐Band–Selected High‐Redshift Galaxy Populations in theAKARINorth Ecliptic Pole Field
Koji Imai, Chris P. Pearson, Hideo Matsuhara, et al. The Astrophysical Journal 683(1) 45 (2008) https://doi.org/10.1086/589633
Formation of Early‐Type Galaxies from Cosmological Initial Conditions
Thorsten Naab, Peter H. Johansson, Jeremiah P. Ostriker and George Efstathiou The Astrophysical Journal 658(2) 710 (2007) https://doi.org/10.1086/510841
Surface density of extremely red objects with R - J ≥ 5
Massive Galaxies and Extremely Red Objects atz= 1–3 in Cosmological Hydrodynamic Simulations: Near‐Infrared Properties
Kentaro Nagamine, Renyue Cen, Lars Hernquist, Jeremiah P. Ostriker and Volker Springel The Astrophysical Journal 627(2) 608 (2005) https://doi.org/10.1086/430699
An overdensity of extremely red objects around faint mid-IR galaxies