Gillian Wilson

Gillian Wilson is a British-American astronomer and cosmologist.

Wilson joined University of California, Merced in October 2022 as Vice Chancellor for Research, Innovation and Economic Development and is also a Professor in the UC Merced Physics Department. She was formerly Professor of Physics and Astronomy at the University of California, Riverside, where she was also Senior Associate Vice Chancellor for Research & Economic Development. Provided by Wikipedia
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  1. 1
    Quantifying the Velocity Anisotropy Profile of Galaxy Clusters Using the Uchuu Cosmological Simulation

    Quantifying the Velocity Anisotropy Profile of Galaxy Clusters Using the Uchuu Cosmological Simulation by Mohamed H. Abdullah, Raouf H. Mabrouk, Tomoaki Ishiyama, Gillian Wilson, Magdy Y. Amin, Elamira Hend Khattab, H. I. Abdel Rahman

    Published 2025-01-01
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  2. 2
    An Indication of Gas Inflow in Clumpy Star-forming Galaxies near z ∼ 1: Lower Gas-phase Metallicities in Clumpy Galaxies Compared to Nonclumpy Galaxies

    An Indication of Gas Inflow in Clumpy Star-forming Galaxies near z ∼ 1: Lower Gas-phase Metallicities in Clumpy Galaxies Compared to Nonclumpy Galaxies by Visal Sok, Adam Muzzin, Pascale Jablonka, Vivian Yun Yan Tan, Z. Cemile Marsan, Danilo Marchesini, Gillian Wilson, Leo Y. Alcorn

    Published 2025-01-01
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  3. 3
    Traversing the Star-forming Main Sequence with Molecular Gas Stacks of z ∼ 1.6 Cluster Galaxies

    Traversing the Star-forming Main Sequence with Molecular Gas Stacks of z ∼ 1.6 Cluster Galaxies by Alex Pigarelli, Allison Noble, Gregory Rudnick, William Cramer, Stacey Alberts, Yannick Bahe, Patrick S. Kamieneski, Sebastian Montaño, Adam Muzzin, Julie Nantais, Sarah Saavedra, Eelco van Kampen, Tracy Webb, Christina C. Williams, Gillian Wilson, H. K. C. Yee

    Published 2025-01-01
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  4. 4
    MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ∼ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 < z < 4

    MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ∼ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 < z < 4 by Ben Forrest, M. C. Cooper, Adam Muzzin, Gillian Wilson, Danilo Marchesini, Ian McConachie, Percy Gomez, Marianna Annunziatella, Z. Cemile Marsan, Joey Braspenning, Wenjun Chang, Gabriella de Lucia, Fabio Fontanot, Michaela Hirschmann, Dylan Nelson, Annalisa Pillepich, Joop Schaye, Stephanie M. Urbano Stawinski, Mauro Stefanon, Lizhi Xie

    Published 2024-01-01
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  5. 5
    MAGAZ3NE: Evidence for Galactic Conformity in z ≳ 3 Protoclusters

    MAGAZ3NE: Evidence for Galactic Conformity in z ≳ 3 Protoclusters by Ian McConachie, Gillian Wilson, Ben Forrest, Z. Cemile Marsan, Adam Muzzin, M. C. Cooper, Marianna Annunziatella, Danilo Marchesini, Percy Gomez, Wenjun Chang, Stephanie M. Urbano Stawinski, Michael McDonald, Tracy Webb, Allison Noble, Brian C. Lemaux, Ekta A. Shah, Priti Staab, Lori M. Lubin, Roy R. Gal

    Published 2024-01-01
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