You can help our author matching system! If you notice any publications incorrectly attributed to this author, please
sign in and mark matches as correct or incorrect.
|
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 |
Zhang Z, Barbary K, Nothaft FA, et al. (2020) Kira: Processing Astronomy Imagery Using Big Data Technology Ieee Transactions On Big Data. 6: 369-381 |
Williams SC, Hook IM, Hayden B, et al. (2020) See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies Monthly Notices of the Royal Astronomical Society. 495: 3859-3880 |
Léget P, Gangler E, Mondon F, et al. (2020) SUGAR: An improved empirical model of Type Ia Supernovae based on spectral features Astronomy and Astrophysics. 636 |
Gonzalez AH, Gettings DP, Brodwin M, et al. (2019) The Massive and Distant Clusters of
WISE
Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at
z
≃ 1 The Astrophysical Journal Supplement Series. 240: 33 |
Kim J, Jee MJ, Perlmutter S, et al. (2019) Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z>1 The Astrophysical Journal. 887: 76 |
Taubenberger S, Floers A, Vogl C, et al. (2019) SN 2012dn from early to late times: 09dc-like supernovae reassessed Monthly Notices of the Royal Astronomical Society. 488: 5473-5488 |
Saunders C, Aldering G, Antilogus P, et al. (2018) SNEMO : Improved Empirical Models for Type Ia Supernovae The Astrophysical Journal. 869: 167-167 |
Foltz R, Wilson G, Muzzin A, et al. (2018) The Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population The Astrophysical Journal. 866: 136 |
Rubin D, Hayden B, Huang X, et al. (2018) The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22 The Astrophysical Journal. 866: 65-65 |