Rachel S. Bezanson, Ph.D.

Affiliations: 
2013 Yale University, New Haven, CT 
 2013-2016 Steward Observatory University of Arizona, Tucson, AZ 
 2016-2017 Princeton University, Princeton, NJ 
 2017- Physics and Astronomy University of Pittsburgh, Pittsburgh, PA, United States 
Website:
https://www.physicsandastronomy.pitt.edu/people/rachel-bezanson
Google:
"Rachel Bezanson"
Bio:

https://rachelbezanson.github.io/images/CV_bezanson.pdf

Mean distance: 17.95
 
SNBCP

Parents

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Pieter G. van Dokkum grad student 2013 Yale
 (Ten Billion Years of Growth: Massive Galaxy Evolution from Structures and Dynamics.)

Children

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Justin Cole research assistant 2020 University of Pittsburgh (Astronomy Tree)
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Publications

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Atek H, Labbé I, Furtak LJ, et al. (2024) Most of the photons that reionized the Universe came from dwarf galaxies. Nature. 626: 975-978
Furtak LJ, Labbé I, Zitrin A, et al. (2024) A high black hole to host mass ratio in a lensed AGN in the early Universe. Nature
Labbé I, van Dokkum P, Nelson E, et al. (2023) A population of red candidate massive galaxies ~600 Myr after the Big Bang. Nature
Whitaker KE, Williams CC, Mowla L, et al. (2021) Quenching of star formation from a lack of inflowing gas to galaxies. Nature. 597: 485-488
Greene JE, Setton D, Bezanson R, et al. (2020) The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuIGG$\vec{L}$E Survey The Astrophysical Journal. 899
Cole J, Bezanson R, Wel Avd, et al. (2020) Stellar Kinematics and Environment at z~0.8 in the LEGA-C Survey:Massive, Slow-Rotators are Built First in Overdense Environments The Astrophysical Journal. 890
Wu P, Wel Avd, Bezanson R, et al. (2020) The Colors and Sizes of Recently Quenched Galaxies: A Result of Compact Starburst before Quenching The Astrophysical Journal. 888: 77
D’Eugenio F, Wel Avd, (吳柏锋) PW, et al. (2020) Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C Monthly Notices of the Royal Astronomical Society. 497: 389-404
Kriek M, Price SH, Conroy C, et al. (2019) Stellar Metallicities and Elemental Abundance Ratios of z ∼ 1.4 Massive Quiescent Galaxies The Astrophysical Journal. 880: L31
Bezanson R, Spilker J, Williams CC, et al. (2019) Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z = 1.522 The Astrophysical Journal. 873: L19
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