Kim-Vy H. Tran, Ph.D.
Affiliations: | 2002 | University of California, Santa Cruz, Santa Cruz, CA, United States |
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"Kim-Vy Tran"Mean distance: 19.4
Parents
Sign in to add mentorGarth D. Illingworth | grad student | 2002 | UC Santa Cruz | |
(Galaxy populations in rich environments.) |
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Publications
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Nanayakkara T, Glazebrook K, Jacobs C, et al. (2024) A population of faint, old, and massive quiescent galaxies at [Formula: see text] revealed by JWST NIRSpec Spectroscopy. Scientific Reports. 14: 3724 |
Glazebrook K, Nanayakkara T, Schreiber C, et al. (2024) A massive galaxy that formed its stars at z ~ 11. Nature |
Esdaile J, Glazebrook K, Labbé I, et al. (2021) Consistent Dynamical and Stellar Masses with Potential Light IMF in Massive Quiescent Galaxies at 3 < z < 4 Using Velocity Dispersions Measurements with MOSFIRE The Astrophysical Journal. 908: L35 |
Gupta A, Tran K, Pillepich A, et al. (2021) MOSEL and IllustrisTNG: Massive Extended Galaxies at z = 2 Quench Later Than Normal-size Galaxies The Astrophysical Journal. 907: 95 |
Schreiber C, Glazebrook K, Papovich C, et al. (2021) A low [CII]/[NII] ratio in the center of a massive galaxy at z = 3.7: Evidence for a transition to quiescence at high redshift? (Corrigendum) Astronomy & Astrophysics. 650: C2 |
Schreiber C, Glazebrook K, Papovich C, et al. (2021) A low [CII]/[NII] ratio in the center of a massive galaxy at z = 3.7: Evidence for a transition to quiescence at high redshift? Astronomy & Astrophysics. 646: A68 |
Tran KH, Forrest B, Alcorn LY, et al. (2020) MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3 |
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 |
Harshan A, Gupta A, Tran K, et al. (2020) ZFIRE: Measuring Electron Density with [O ii] as a Function of Environment at z = 1.62 The Astrophysical Journal. 892: 77 |
Nanayakkara T, Brinchmann J, Glazebrook K, et al. (2020) Reconstructing the Observed Ionizing Photon Production Efficiency at z ∼ 2 Using Stellar Population Models The Astrophysical Journal. 889: 180 |