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
The NuSTAR Extragalactic Survey: A First Sensitive Look at the High-energy Cosmic X-Ray Background Population
David M. Alexander,D. Stern,A. Del Moro,George B. Lansbury,Roberto J. Assef,James Aird,Marco Ajello,David R. Ballantyne,Franz E. Bauer,S. E. Boggs,W. N. Brandt,Finn Erland Christensen,F. Civano,Andrea Comastri,W. W. Craig,Martin Elvis,Brian W. Grefenstette,C. J. Hailey,Fiona A. Harrison,Ryan C. Hickox,B. Luo,K. K. Madsen,James Mullaney,M. Perri,Simonetta Puccetti,Cristian Saez,Ezequiel Treister,C. M. Urry,W. W. Zhang,Carrie Bridge,Peter Eisenhardt,Anthony H. Gonzalez,Sarah H. Miller,Chao-Wei Tsai +33 more
TL;DR: In this article, the authors report on the first 10 identifications of sources serendipitously detected by the Nuclear Spectroscopic Telescope Array (NuSTAR) to provide the first sensitive census of the cosmic X-ray background source population at ≳10 keV.
Journal ArticleDOI
Rest-frame Ultraviolet-to-Optical Properties of Galaxies at z ~ 6 and 5 in the Hubble Ultra Deep Field: from Hubble to Spitzer
Haojing Yan,Mark Dickinson,Daniel Stern,Peter Eisenhardt,Ranga-Ram Chary,Mauro Giavalisco,Henry C. Ferguson,Stefano Casertano,Christopher J. Conselice,Casey Papovich,William T. Reach,Norman A. Grogin,Leonidas A. Moustakas,Masami Ouchi +13 more
TL;DR: In this paper, the authors used data from the first epoch of observations with the IRAC/Spitzer for the GOODS to detect and study a collection of LBGs at z ~ 6 to 5 in the HUDF, six of which have spectroscopic confirmation.
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The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years
Stacey Alberts,Alexandra Pope,Mark Brodwin,David W. Atlee,Yen-Ting Lin,Arjun Dey,Peter Eisenhardt,D. Gettings,Anthony H. Gonzalez,Buell T. Jannuzi,Conor L. Mancone,John Moustakas,Gregory F. Snyder,S. Adam Stanford,Daniel Stern,Benjamin J. Weiner,Gregory R. Zeimann +16 more
TL;DR: In this paper, the authors compare the star formation activity in cluster galaxies to the field from z = 0.3-1.5 using SPIRE 250$\mu$m imaging.
Journal ArticleDOI
Clustering of obscured and unobscured quasars in the Bootes field: Placing rapidly growing black holes in the cosmic web
Ryan C. Hickox,Adam D. Myers,Mark Brodwin,David M. Alexander,William R. Forman,Christine Jones,Stephen S. Murray,Michael J. I. Brown,Richard J. Cool,Roberto J. Assef,Christopher S. Kochanek,Arjun Dey,Buell T. Jannuzi,Daniel J. Eisenstein,Peter Eisenhardt,Varoujan Gorjian,Daniel Stern,Emeric Le Floc'h,Nelson Caldwell,Andy D. Goulding,James Mullaney +20 more
TL;DR: In this paper, the authors present the first measurement of the spatial clustering of mid-infrared selected obscured and unobscured quasars, using a sample in the redshift range 0.7 < z < 1.
Journal ArticleDOI
Evolution of Infrared-selected Galaxies in Z approximately 0.4 Clusters
TL;DR: In this paper, a wide-field optical and near-IR (JHK) imaging is presented for two rich galaxy clusters: Abell~370 at 0.374 and Abell ~851 (Cl0939+47), where the intrinsic scatter of the known E/S0s about their optical-K$ color-mag relation is small.