Saul Perlmutter
Affiliations: | 2004- | Physics | University of California, Berkeley, Berkeley, CA, United States |
Website:
http://www.nobelprize.org/nobel_prizes/physics/laureates/2011/perlmutter-bio.htmlGoogle:
"Saul Perlmutter"Bio:
http://www.nasonline.org/member-directory/members/3007673.html
http://physics.berkeley.edu/people/faculty/saul-perlmutter
https://history.aip.org/phn/11608006.html
https://inspirehep.net/record/993746?ln=en
https://books.google.com/books?id=ueFIAQAAMAAJ
The Nobel Prize in Physics 2011 was divided, one half awarded to Saul Perlmutter, the other half jointly to Brian P. Schmidt and Adam G. Riess "for the discovery of the accelerating expansion of the Universe through observations of distant supernovae".
Mean distance: 14.01 | S | N | B | C | P |
Parents
Sign in to add mentor| Richard A. Muller | grad student | 1986 | UC Berkeley | |
| (An Astronomic Search for a Stellar Companion to the Sun) | ||||
Children
Sign in to add trainee| Radhika Rawat | research assistant | 2014-2015 | Lawrence Berkeley National Lab, UC Berkeley (Neurotree) |
| David A Rubin | grad student | UC Berkeley/LBNL (Neurotree) | |
| William M. Wood-Vasey | grad student | UC Berkeley | |
| Alexander J. Conley | grad student | 2005 | UC Berkeley |
| Roland De Putter | grad student | 2010 | UC Berkeley |
| Kyle H. Barbary | grad student | 2011 | UC Berkeley |
| Michael J. Childress | grad student | 2011 | UC Berkeley |
| Jessica A. Kirkpatrick | grad student | 2012 | UC Berkeley |
| Joshua E. Meyers | grad student | 2012 | UC Berkeley |
| Hannah K. Fakhouri | grad student | 2013 | UC Berkeley |
| Antonella Palmese | post-doc | (Astronomy Tree) | |
| Brian T. Hayden | post-doc | 2013-2018 | LBNL |
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Publications
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| 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 |