Gillian Wilson
Affiliations: | Physics | University of California, Riverside, Riverside, CA, United States |
Area:
Astronomy and Astrophysics, Astrophysics PhysicsGoogle:
"Gillian Wilson"Mean distance: (not calculated yet)
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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 |
| Finner K, Jee MJ, Webb T, et al. (2020) Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z = 1.71 with Infrared Weak Lensing The Astrophysical Journal. 893: 10 |
| Matharu J, Muzzin A, Brammer GB, et al. (2020) HST/WFC3 grism observations of z ∼ 1 clusters: evidence for evolution in the mass–size relation of quiescent galaxies from post-starburst galaxies Monthly Notices of the Royal Astronomical Society. 493: 6011-6032 |
| 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 |
| 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 |
| Noble AG, Muzzin A, McDonald M, et al. (2019) Resolving CO (2−1) in z ∼ 1.6 Gas-rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping The Astrophysical Journal. 870: 56 |
| Trudeau A, Webb T, Hlavacek-Larrondo J, et al. (2019) Multiwavelength radio observations of a brightest cluster galaxy at z = 1.71: detection of a modest active galactic nucleus and evidence for extended star formation Monthly Notices of the Royal Astronomical Society. 487: 1210-1217 |
| Abdullah MH, Wilson G, Klypin A. (2018) GalWeight: A New and Effective Weighting Technique for Determining Galaxy Cluster and Group Membership The Astrophysical Journal. 861: 22 |