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Ben Forrest

Affiliations: 
Texas A & M University, College Station, TX, United States 
Area:
Galaxy Evolution
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"Ben Forrest"
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Kim-Vy H. Tran grad student

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Publications

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Forrest B, Annunziatella M, Wilson G, et al. (2020) An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models The Astrophysical Journal. 890
Tran KH, Forrest B, Alcorn LY, et al. (2020) MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3The Astrophysical Journal. 898: 45
Gupta A, Tran K, Cohn J, et al. (2020) MOSEL Survey: Tracking the Growth of Massive Galaxies at 2 < z < 4 Using Kinematics and the IllustrisTNG Simulation The Astrophysical Journal. 893: 23
Old LJ, Balogh ML, van der Burg RFJ, et al. (2020) The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5 Monthly Notices of the Royal Astronomical Society. 493: 5987-6000
Webb K, Balogh ML, Leja J, et al. (2020) The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z > 1 Monthly Notices of the Royal Astronomical Society
Burg RFJVD, Rudnick G, Balogh ML, et al. (2020) The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching Astronomy and Astrophysics. 638
Alcorn LY, Gupta A, Tran K, et al. (2019) A Tale of Two Clusters: An Analysis of Gas-phase Metallicity and Nebular Gas Conditions in Proto-cluster Galaxies at z ∼ 2 The Astrophysical Journal. 883: 153
Chan JCC, Wilson G, Rudnick G, et al. (2019) The Rest-frame H-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 < z < 1.3 The Astrophysical Journal. 880: 119
Cohn JH, Leja J, Tran KH, et al. (2018) zfourge: Extreme 5007 Å Emission May Be a Common Early-lifetime Phase for Star-forming Galaxies at z > 2.5 The Astrophysical Journal. 869: 141
Forrest B, Tran KH, Broussard A, et al. (2018) ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1 < z < 4 The Astrophysical Journal. 863: 131
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