P
Peter Eisenhardt
Researcher at California Institute of Technology
Publications - 330
Citations - 43497
Peter Eisenhardt is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 93, co-authored 324 publications receiving 39810 citations. Previous affiliations of Peter Eisenhardt include University of California, Davis & National Science Foundation.
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Journal ArticleDOI
The Massive and Distant Clusters of WISE Survey: MOO J1142+1527, A 10$^{15}$ M$_\odot$ Galaxy Cluster at z=1.19
Anthony H. Gonzalez,Bandon Decker,Mark Brodwin,Peter Eisenhardt,Daniel P. Marrone,S. A. Stanford,Daniel Stern,Dominika Wylezalek,Greg Aldering,Zubair Abdulla,Kyle Boone,John E. Carlstrom,Parker Fagrelius,D. Gettings,Christopher Greer,Brian Hayden,Erik M. Leitch,Yen-Ting Lin,Adam Mantz,Stephen Muchovej,Saul Perlmutter,Gregory R. Zeimann +21 more
TL;DR: In this paper, a massive galaxy cluster known as MOO J1142+1527 was confirmed to lie at the Sunyaev-Zel'dovich (SZ) decrement at 13.2$\sigma using the Combined Array for Research in Millimeter-wave Astronomy (CARM).
Journal ArticleDOI
The Massive and Distant Clusters of WISE Survey: MOO J1142+1527, a 10^(15) M_⊙ Galaxy Cluster at z = 1.19
Anthony H. Gonzalez,B. Decker,Mark Brodwin,Peter Eisenhardt,Daniel P. Marrone,S. A. Stanford,S. A. Stanford,Daniel Stern,Dominika Wylezalek,Greg Aldering,Zubair Abdulla,Kyle Boone,Kyle Boone,John E. Carlstrom,Parker Fagrelius,Parker Fagrelius,D. Gettings,Christopher Greer,Brian Hayden,Brian Hayden,Erik M. Leitch,Yen-Ting Lin,Adam Mantz,Stephen Muchovej,Saul Perlmutter,Saul Perlmutter,Gregory R. Zeimann +26 more
TL;DR: In this paper, a massive galaxy cluster known as MOO J1142+1527 was confirmed to lie at z = 1.19, and using the Combined Array for Research in Millimeter-wave Astronomy, robustly detect the Sunyaev-Zel'dovich (SZ) decrement at 13.2σ.
Journal ArticleDOI
The formation history of massive cluster galaxies as revealed by CARLA
E. A. Cooke,Nina A. Hatch,Alessandro Rettura,Dominika Wylezalek,Audrey Galametz,D. Stern,Mark Brodwin,Stuart I. Muldrew,Omar Almaini,Christopher J. Conselice,Peter Eisenhardt,William G. Hartley,Matt J. Jarvis,Matt J. Jarvis,Nick Seymour,S. A. Stanford +15 more
TL;DR: In this paper, the authors used a sample of 37 of the densest clusters and protoclusters across 1.3 ≤ z ≤ 3.2 from the Clusters Around Radio-Loud AGN (CARLA) survey to study the formation of massive cluster galaxies.
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MIPS J142824.0+352619: a hyperluminous starburst galaxy at z = 1.325
Colin Borys,Andrew W. Blain,Arjun Dey,E. Le Floc'h,Buell T. Jannuzi,V. Barnard,C. Bian,Mark Brodwin,Karín Menéndez-Delmestre,David R. Thompson,Kate Brand,Michael J. I. Brown,C. D. Dowell,C. D. Dowell,Peter Eisenhardt,Duncan Farrah,Duncan Farrah,David T. Frayer,James L. Higdon,Sarah J.U. Higdon,Thomas G. Phillips,B. T. Soifer,Daniel Stern,Daniel W. Weedman +23 more
TL;DR: In this article, the authors used the SHARC-II camera at the Caltech Submillimeter Observatory to obtain 350 μm images of sources detected with the MIPS instrument on Spitzer, and discovered a remarkable object at z = 1.325 ± 0.002 with an apparent far-infrared luminosity of 3.2(± 0.7) × 1013 L
Journal ArticleDOI
The Hubble Space Telescope Cluster Supernova Survey: VI. The Volumetric Type Ia Supernova Rate
Kyle Barbary,Greg Aldering,Rahman Amanullah,M. Brodwin,Natalia Connolly,Kyle S. Dawson,Mamoru Doi,Peter Eisenhardt,L. Faccioli,Vitaliy Fadeyev,H. K. Fakhouri,A. S. Fruchter,David G. Gilbank,Michael D. Gladders,G. Goldhaber,A. Goobar,Takashi Hattori,Eric Hsiao,Xiaosheng Huang,Yutaka Ihara,Nobunari Kashikawa,Benjamin P. Koester,Kohki Konishi,M. Kowalski,C. Lidman,Lori M. Lubin,J. Meyers,Tomoki Morokuma,Takeshi Oda,Nino Panagia,Saul Perlmutter,Marc Postman,P. Ripoche,Piero Rosati,David Rubin,David J. Schlegel,A. L. Spadafora,S. A. Stanford,M. Strovink,Nao Suzuki,Naohiro Takanashi,Kouichi Tokita,Naoki Yasuda,Supernova Cosmology +43 more
TL;DR: In this article, the authors presented a measurement of the volumetric Type Ia supernova (SN Ia) rate out to z ~ 1.6 from the Hubble Space Telescope Cluster Supernova Survey.