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.
Papers
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Journal ArticleDOI
Hubble Space Telescope Imaging Polarimetry of the Gravitational Lens FSC 10214+4724
Hien Nguyen,Peter Eisenhardt,Michael W. Werner,Robert W. Goodrich,David W. Hogg,Lee Armus,B. T. Soifer,G. Neugebauer +7 more
TL;DR: In this article, the authors presented an imaging polarimetry of the extremely luminous, redshift 2.3 IRAS source FSC 10214+4724, which was obtained with HST's Faint Object Camera in the F437M filter.
Journal ArticleDOI
NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-Selected Quasars at z ~ 2
D. Stern,George B. Lansbury,Roberto J. Assef,W. N. Brandt,David M. Alexander,David R. Ballantyne,Mislav Baloković,Dominic J. Benford,Andrew Blain,S. E. Boggs,Carrie Bridge,Murray Brightman,F. E. Christensen,Andrea Comastri,William W. Craig,A. Del Moro,Peter Eisenhardt,Poshak Gandhi,Roger L. Griffith,C. J. Hailey,Fiona A. Harrison,Ryan C. Hickox,Thomas H. Jarrett,Michael Koss,S. E. Lake,Stephanie M. LaMassa,B. Luo,C. W. Tsai,Dominic J. Walton,Edward L. Wright,Jingwen Wu,Lin Yan,W. W. Zhang +32 more
TL;DR: In this article, a NuSTAR and XMM-Newton program has observed a sample of three extremely luminous, heavily obscured WISE-selected AGN at z~2 in a broad X-ray band (0.1 - 79 keV).
Posted Content
A measurement of the intrahalo light fraction with near-infrared background anisotropies
Asantha Cooray,Joseph Smidt,Francesco De Bernardis,Yan Gong,Daniel Stern,Matthew L. N. Ashby,Peter Eisenhardt,Christopher C. Frazer,Anthony H. Gonzalez,Christopher S. Kochanek,Szymon Kozłowski,Edward L. Wright +11 more
TL;DR: In this paper, the authors measured the anisotropy power spectrum from subarcminute to one degree angular scales and found the clustering amplitude to be larger than the model predictions involving the two existing explanations.
Posted Content
Results from the Wide-field Infrared Survey Explorer (WISE) Future Uses Session at the WISE at 5 Meeting
Jacqueline K. Faherty,K. Alatalo,L. D. Anderson,Roberto J. Assef,Daniella C. Bardalez Gagliuffi,Megan Barry,Dominic J. Benford,Maciej Bilicki,Ben Burningham,Damian J. Christian,Michael C. Cushing,Peter Eisenhardt,Martin Elvisx,Sergio Fajardo-Acosta,Douglas P. Finkbeiner,William J. Fischer,William J. Forrest,John W. Fowler,Jonathan P. Gardner,Christopher R. Gelino,Gorjian,Carl J. Grillmair,Mariusz Gromadzki,Kendall Paige Hall,Zeljko Ivezic,Natsuko Izumi,J. Davy Kirkpatrick,András Kovács,Dustin Lang,David Leisawitz,Fengchuan Liu,A. K. Mainzer,Katarzyna Małek,Gábor Marton,Frank J. Masci,Ian S. McLean,Aaron Meisner,R. Nikutta,Deborah Padgett,Rahul Patel,Luisa Rebull,Jeffrey A. Rich,F. A. Ringwald,Marvin Rose,Adam C. Schneider,Keivan G. Stassun,Daniel Stern,Chao-Wei Tsai,Feige Wang,Madalyn E. Weston,Edward L.,Wright,Jingwen Wu,Jinyi Yang +53 more
TL;DR: An interactive session exploring the future uses of the Wide-field Infrared Survey Explorer (WISE) data found that complementing WISE/NEOWISE data with cross-correlated multiwavelength surveys would be highly beneficial for all future mission goals.
Journal ArticleDOI
Measuring the total infrared light from galaxy clusters at z = 0.5–1.6: connecting stellar populations to dusty star formation
Stacey Alberts,Kyoung-Soo Lee,Alexandra Pope,Mark Brodwin,Yi-Kuan Chiang,Jed McKinney,Rui Xue,Yun Huang,Michael J. I. Brown,Arjun Dey,Peter Eisenhardt,Buell T. Jannuzi,Roxana Popescu,Vandana Ramakrishnan,S. A. Stanford,Benjamin J. Weiner +15 more
TL;DR: In this paper, the total light stacking technique was used to reveal the total cluster IR emission, including low mass members and potential intracluster dust, in 232 massive (log M200/Msun~13.8) clusters across multiple z bins, typically at >5sigma.