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Saul Perlmutter, UC Berkeley/Lawrence Berkeley Lab (Nobel Prize in Physics, 2011)

There are 55 publications in this collection, published between 1998 and 2022. Showing 1 - 50.

Briday, M; Rigault, M; Graziani, R; Copin, Y; Aldering, G; Amenouche, M et al.: Accuracy of environmental tracers and consequences for determining the Type Ia supernova magnitude step, 2022

Boone, K; Aldering, G; Antilogus, P; Aragon, C; Bailey, S; Baltay, C et al.: The Twins Embedding of Type Ia Supernovae. I. The Diversity of Spectra at Maximum Light, 2021

Boone, K; Aldering, G; Antilogus, P; Aragon, C; Bailey, S; Baltay, C et al.: The Twins Embedding of Type Ia Supernovae. II. Improving Cosmological Distance Estimates, 2021

Nicolas, N; Rigault, M; Copin, Y; Graziani, R; Aldering, G; Briday, M et al.: Redshift evolution of the underlying type Ia supernova stretch distribution, 2021

Rubin, David; Cikota, Aleksandar; Aldering, Greg; Fruchter, Andy; Perlmutter, Saul; Sako, Masao: Going Forward with the Nancy Grace Roman Space Telescope Transient Survey: Validation of Precision Forward-modeling Photometry for Undersampled Imaging, 2021

Hsiao, EY; Hoeflich, P; Ashall, C; Lu, J; Contreras, C; Burns, CR et al.: Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events* * This paper includes data gathered with the 1 m Swope and 2.5 m du Pont telescopes at Las Campanas Observatory, Chile, and the Nordic Optical Telescope at the Observatorio del Roque de los Muchachos, La Palma, Spain., 2020

Léget, PF; Gangler, E; Mondon, F; Aldering, G; Antilogus, P; Aragon, C et al.: SUGAR: An improved empirical model of Type Ia supernovae based on spectral features, 2020

Rigault, M; Brinnel, V; Aldering, G; Antilogus, P; Aragon, C; Bailey, S et al.: Strong dependence of Type Ia supernova standardization on the local specific star formation rate⋆, 2020

Gonzalez, AH; Gettings, DP; Brodwin, M; Eisenhardt, PRM; Stanford, SA; Wylezalek, D et al.: The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z ≃ 1, 2019

Hsiao, EY; Phillips, MM; Marion, GH; Kirshner, RP; Morrell, N; Sand, DJ et al.: Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program* ∗ This paper includes data gathered with the 6.5-m Magellan telescopes at Las Campanas Observatory, Chile., 2019

Kim, J; Jee, MJ; Perlmutter, S; Hayden, B; Rubin, D; Huang, X et al.: Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z > 1, 2019

Phillips, MM; Contreras, Carlos; Hsiao, EY; Morrell, Nidia; Burns, Christopher R; Stritzinger, Maximilian et al.: Carnegie Supernova Project-II: Extending the Near-infrared Hubble Diagram for Type Ia Supernovae to z ∼ 0.1∗ ∗ This paper includes data gathered with the 6.5 meter Magellan telescopes at Las Campanas Observatory, Chile., 2019

Taubenberger, S; Floers, A; Vogl, C; Kromer, M; Spyromilio, J; Aldering, G et al.: SN 2012dn from early to late times: 09dc-like supernovae reassessed, 2019

Boone, K; Aldering, G; Copin, Y; Dixon, S; Domagalski, RS; Gangler, E et al.: A binary offset effect in CCD readout and its impact on astronomical data, 2018

Foltz, R; Wilson, G; Muzzin, A; Cooper, MC; Nantais, J; van der Burg, RFJ et al.: The Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population, 2018

Léget, P-F; Pruzhinskaya, MV; Ciulli, A; Gangler, E; Aldering, G; Antilogus, P et al.: Correcting for peculiar velocities of Type Ia supernovae in clusters of galaxies, 2018

Nordin, J; Aldering, G; Antilogus, P; Aragon, C; Bailey, S; Baltay, C et al.: Understanding type Ia supernovae through their U-band spectra★, 2018

Rubin, D; Hayden, B; Huang, X; Aldering, G; Amanullah, R; Barbary, K et al.: The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22, 2018

Saunders, C; Aldering, G; Antilogus, P; Bailey, S; Baltay, C; Barbary, K et al.: SNEMO: Improved Empirical Models for Type Ia Supernovae, 2018

Wu, Jingwen; Jun, Hyunsung D; Assef, Roberto J; Tsai, Chao-Wei; Wright, Edward L; Eisenhardt, Peter RM et al.: Eddington-limited Accretion in z ∼ 2 WISE-selected Hot, Dust-obscured Galaxies, 2018

Delahaye, AG; Webb, TMA; Nantais, J; DeGroot, A; Wilson, G; Muzzin, A et al.: Galaxy Merger Candidates in High-redshift Cluster Environments, 2017

Huang, X; Raha, Z; Aldering, G; Antilogus, P; Bailey, S; Baltay, C et al.: The Extinction Properties of and Distance to the Highly Reddened Type IA Supernova 2012cu, 2017

Jee, M James; Ko, Jongwan; Perlmutter, Saul; Gonzalez, Anthony; Brodwin, Mark; Linder, Eric et al.: First Weak-lensing Results from “See Change”: Quantifying Dark Matter in the Two z ≳ 1.5 High-redshift Galaxy Clusters SPT-CL J2040–4451 and IDCS J1426+3508, 2017

Lombardo, S; Küsters, D; Kowalski, M; Aldering, G; Antilogus, P; Bailey, S et al.: SCALA: In situ calibration for integral field spectrographs, 2017

Mitsuda, K; Doi, M; Morokuma, T; Suzuki, N; Yasuda, N; Perlmutter, S et al.: Isophote Shapes of Early-Type Galaxies in Massive Clusters at z ∼ 1 and 0, 2017

Noble, AG; McDonald, M; Muzzin, A; Nantais, J; Rudnick, G; van Kampen, E et al.: ALMA Observations of Gas-rich Galaxies in z ∼ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments, 2017

Fakhouri, HK; Boone, K; Aldering, G; Antilogus, P; Aragon, C; Bailey, S et al.: IMPROVING COSMOLOGICAL DISTANCE MEASUREMENTS USING TWIN TYPE IA SUPERNOVAE, 2015

Feindt, U; Kerschhaggl, M; Kowalski, M; Aldering, G; Antilogus, P; Aragon, C et al.: Measuring cosmic bulk flows with Type Ia supernovae from the Nearby Supernova Factory (Corrigendum), 2015

Kim, AG; Padmanabhan, N; Aldering, G; Allen, SW; Baltay, C; Cahn, RN et al.: Distance probes of dark energy, 2015

Saunders, C; Aldering, G; Antilogus, P; Aragon, C; Bailey, S; Baltay, C et al.: TYPE Ia SUPERNOVA DISTANCE MODULUS BIAS AND DISPERSION FROM K-CORRECTION ERRORS: A DIRECT MEASUREMENT USING LIGHT CURVE FITS TO OBSERVED SPECTRAL TIME SERIES, 2015

Zhang, Zhao; Barbary, Kyle; Nothaft, Frank Austin; Sparks, Evan; Zahn, Oliver; Franklin, Michael J et al.: Scientific Computing Meets Big Data Technology: An Astronomy Use Case, 2015

Scalzo, R; Aldering, G; Antilogus, P; Aragon, C; Bailey, S; Baltay, C et al.: Type Ia supernova bolometric light curves and ejected mass estimates from the Nearby Supernova Factory, 2014

Rubin, D; Linder, EV; Kowalski, M; Aldering, G; Amanullah, R; Barbary, K et al.: LOOKING BEYOND LAMBDA WITH THE UNION SUPERNOVA COMPILATION, 2009

Santos, JS; Rosati, P; Gobat, R; Lidman, C; Dawson, K; Perlmutter, S et al.: Multiwavelength observations of a rich galaxy cluster at z 1*, 2009

Kowalski, M; Rubin, D; Aldering, G; Agostinho, RJ; Amadon, A; Amanullah, R et al.: Improved Cosmological Constraints from New, Old, and Combined Supernova Data Sets, 2008

Morokuma, Tomoki; Doi, Mamoru; Yasuda, Naoki; Akiyama, Masayuki; Sekiguchi, Kazuhiro; Furusawa, Hisanori et al.: The Subaru/XMM-Newton Deep Survey (SXDS). V. Optically Faint Variable Object Survey**Based in part on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. Based on observations (program GN-2002B-Q-30) obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (US), the Particle Physics and Astronomy Research Council (UK), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), CNPq (Brazil), and CONICET (Argentina)., 2008

Aldering, Greg; Kim, Alex G; Kowalski, Marek; Linder, Eric V; Perlmutter, Saul: Snapping supernovae at z > 1.7, 2007

Garavini, G; Folatelli, G; Nobili, S; Aldering, G; Amanullah, R; Antilogus, P et al.: Quantitative comparison between type Ia supernova spectra at low and high redshifts: a case study, 2007

Neill, James D; Sullivan, M; Balam, D; Pritchet, CJ; Howell, DA; Perrett, K et al.: The Supernova Type Ia Rate Evolution with SNLS, 2007

Conley, A; Goldhaber, G; Wang, L; Aldering, G; Amanullah, R; Commins, ED et al.: Measurement of Ωm, ΩΛ from a Blind Analysis of Type Ia Supernovae with CMAGIC: Using Color Information to Verify the Acceleration of the Universe, 2006

Neill, JD; Sullivan, M; Balam, D; Pritchet, CJ; Howell, DA; Perrett, K et al.: The Type Ia Supernova Rate at z ≈ 0.5 from the Supernova Legacy Survey**Based on observations obtained with MegaPrime/MegaCam, a joint project of the Canada-France-Hawaii Telescope (CFHT) and CEA/DAPNIA, at CFHT, which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. This work is also based on observations obtained at the European Southern Observatory using the Very Large Telescope on the Cerro Paranal (ESO Large Program 171.A-0486), and on observations (programs GN-2004A-Q-19, GS-2004A-Q-11, GN-2003B-Q-9, and GS-2003B-Q-8) obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the National Science Foundation (NSF) on behalf of the Gemini partnership: the NSF (United States), the Particle Physics and Astronomy Research Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), CNPq (Brazil), and CONICET (Argentina). This work is also based on observations obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation., 2006

Sullivan, M; Howell, DA; Perrett, K; Nugent, PE; Astier, P; Aubourg, E et al.: Photometric Selection of High-Redshift Type Ia Supernova Candidates, 2006

Sullivan, M; Le Borgne, D; Pritchet, CJ; Hodsman, A; Neill, JD; Howell, DA et al.: Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies, 2006

Foley, Ryan J; Filippenko, Alexei V; Leonard, Douglas C; Riess, Adam G; Nugent, Peter; Perlmutter, Saul: A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex, 2005

Hook, IM; Howell, DA; Aldering, G; Amanullah, R; Burns, MS; Conley, A et al.: Spectra of High-Redshift Type Ia Supernovae and a Comparison with Their Low-Redshift Counterparts**Much of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. Also based in part on observations made with the European Southern Observatory telescopes (ESO programs 58.A-0745 and 59.A-0745)., 2005

Lidman, C; Howell, DA; Folatelli, G; Garavini, G; Nobili, S; Aldering, G et al.: Spectroscopic confirmation of high-redshift supernovae with the ESO VLT ***, 2005

Nobili, S; Amanullah, R; Garavini, G; Goobar, A; Lidman, C; Stanishev, V et al.: Restframe I-band Hubble diagram for type Ia supernovae up to redshift z 0.5, 2005

Knop, RA; Aldering, G; Amanullah, R; Astier, P; Blanc, G; Burns, MS et al.: New Constraints on ΩM, ΩΛ, and w from an Independent Set of 11 High-Redshift Supernovae Observed with the Hubble Space Telescope**Based in part on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs GO-7336, GO-7590, and GO-8346. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. Based in part on observations obtained at the WIYN Observatory, which is a joint facility of the University of Wisconsin at Madison, Indiana University, Yale University, and the National Optical Astronomy Observatory. Based in part on observations made with the European Southern Observatory telescopes (ESO programs 60.A-0586 and 265.A-5721). Based in part on observations made with the Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, le Centre National de la Recherche Scientifique de France, and the University of Hawaii., 2003

Sullivan, M; Ellis, RS; Aldering, G; Amanullah, R; Astier, P; Blanc, G et al.: The Hubble diagram of type Ia supernovae as a function of host galaxy morphology, 2003

Wang, Lifan; Baade, Dietrich; Höflich, Peter; Khokhlov, Alexei; Wheeler, J Craig; Kasen, D et al.: Spectropolarimetry of SN 2001el in NGC 1448: Asphericity of a Normal Type Ia Supernova**Based on observations collected at the European Southern Observatory, Chile (ESO Programme 68.D-0571(A)., 2003

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