Tiantian Yuan, Ph.D.
Affiliations: | 2012 | University of Hawai'i at Manoa, Honolulu, HI |
Area:
Astronomy and Astrophysics, Astrophysics PhysicsGoogle:
"Tiantian Yuan"Parents
Sign in to add mentor| Lisa Kewley | grad student | 2012 | University of Hawai'i at Manoa | |
| (Using strong gravitationally lensed galaxies to probe the metallicity history of star-forming galaxies between redshift 1 and 3.) | ||||
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Publications
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| Tran KH, Forrest B, Alcorn LY, et al. (2020) MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3 |
| Cameron AJ, Jones T, Yuan T, et al. (2019) Prospects for Extending the Mass-Metallicity Relation to Low Mass at High Redshift: A Case Study at z ∼ 1 The Astrophysical Journal. 882: 116-116 |
| 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 |
| Gupta A, Yuan T, Torrey P, et al. (2018) Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations Monthly Notices of the Royal Astronomical Society: Letters. 477: L35-L39 |
| Glazebrook K, Schreiber C, Labbé I, et al. (2017) A massive, quiescent galaxy at a redshift of 3.717. Nature. 544: 71-74 |
| Yuan T, Richard J, Gupta A, et al. (2017) The Most Ancient Spiral Galaxy: A 2.6-Gyr-old Disk with a Tranquil Velocity Field The Astrophysical Journal. 850: 61 |
| Gupta A, Yuan T, Martizzi D, et al. (2017) Survival of Massive Star-forming Galaxies in Cluster Cores Drives Gas-phase Metallicity Gradients: The Effects of Ram Pressure Stripping The Astrophysical Journal. 842: 75 |
| Straatman CMS, Glazebrook K, Kacprzak GG, et al. (2017) ZFIRE: The Evolution of the Stellar Mass Tully–Fisher Relation to Redshift ∼2.2 The Astrophysical Journal. 839: 57 |
| Tran KH, Alcorn LY, Kacprzak GG, et al. (2017) ZFIRE: SIMILAR STELLAR GROWTH IN Hα-EMITTING CLUSTER AND FIELD GALAXIES ATz∼ 2 The Astrophysical Journal. 834: 101 |
| Federrath C, Salim DM, Medling AM, et al. (2017) The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates Monthly Notices of the Royal Astronomical Society. 468: 3965-3978 |