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
A catalog of mid-infrared sources in the Extended Groth Strip
Pauline Barmby,J. S. Huang,Matthew L. N. Ashby,Peter Eisenhardt,Giovanni G. Fazio,Edward L. Wright +5 more
TL;DR: The Extended Groth Strip (EGS) is one of the premier fields for extragalactic deep surveys as mentioned in this paper, and the catalog comprises 57434 objects detected at 3.6 um, with 84, 28, and 24% also detected at 4.5, 5.8, and 8.0 um.
Journal ArticleDOI
Origin of the 12 µm Emission Across Galaxy Populations from WISE and SDSS Surveys
Emilio Donoso,Lin Yan,Chao-Wei Tsai,Peter Eisenhardt,D. Stern,Roberto J. Assef,David Leisawitz,Thomas H. Jarrett,S. A. Stanford +8 more
TL;DR: In this article, the authors identify which stellar populations are responsible for most of the 12µm emission in star-forming galaxies from the blue sequence, with total IR lµminosities in the range ~10^8-10^(12) L_⊙.
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A New Population of High Redshift, Dusty Lyman-Alpha Emitters and Blobs Discovered by WISE
Carrie Bridge,Andrew Blain,Colin Borys,Sara Petty,Dominic J. Benford,Peter Eisenhardt,Duncan Farrah,Roger L. Griffith,Thomas H. Jarrett,S. Adam Stanford,Daniel Stern,Chao-Wei Tsai,Edward L. Wright,Jingwen Wu +13 more
TL;DR: In this paper, the authors reported a new technique to select 1.6 10−13−14L_sun (1.6 L_sun) and warm colors, typically larger than submillimeter-selected galaxies (SMGs) and dust-obscured galaxies (DOGs), which are commonly associated with the dust being energized by intense AGN activity.
Journal ArticleDOI
Evolution of the Color-Magnitude Relation in High-Redshift Clusters: Blue Early-Type Galaxies and Red Pairs in RDCS J0910+5422
Simona Mei,John P. Blakeslee,S. A. Stanford,S. A. Stanford,Bradford P. Holden,Piero Rosati,V. Strazzullo,Nicole Homeier,Marc Postman,Marc Postman,M. Franx,Alessandro Rettura,Alessandro Rettura,Holland C. Ford,Garth D. Illingworth,Stefano Ettori,Rychard Bouwens,Ricardo Demarco,André R. Martel,Mark Clampin,George F. Hartig,Peter Eisenhardt,David R. Ardila,F. Bartko,Narciso Benítez,Larry Bradley,Tom Broadhurst,Robert A. Brown,C. J. Burrows,E. S. Cheng,Nicholas Cross,Paul D. Feldman,David A. Golimowski,Tomotsugu Goto,Caryl Gronwall,Leopoldo Infante,Randy A. Kimble,John Krist,Michael Lesser,Felipe Menanteau,Gerhardt R. Meurer,G. K. Miley,V. Motta,Marco Sirianni,William B. Sparks,Hien D. Tran,Zlatan Tsvetanov,R. L. White,W. Zheng +48 more
TL;DR: The color-magnitude relation for the RDCS J0910+5422 cluster of galaxies at redshift z = 1.106 has been determined for the first time in this article.
Journal ArticleDOI
The Detection and Photometric Redshift Determination of Distant Galaxies using SIRTF's Infrared Array Camera
Chris Simpson,Peter Eisenhardt +1 more
TL;DR: In this paper, the authors investigate the ability of the Space Infrared Telescope Facility's Infrared Array Camera to detect distant (z~3) galaxies and measure their photometric redshifts.