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 Rest-Frame K-Band Luminosity Function of Galaxies in Clusters to z = 1.3
Roberto De Propris,S. A. Stanford,S. A. Stanford,Peter Eisenhardt,Peter Eisenhardt,Brad Holden,Piero Rosati +6 more
TL;DR: In this article, the rest-frame K-band luminosity function for galaxies in 32 clusters at 0.6 < z < 1.3 was derived using deep 3.6 and 4.5 μm imaging from the Spitzer Space Telescope Infrared Array Camera.
Journal ArticleDOI
The exemplar t8 subdwarf companion of wolf 1130
Gregory N. Mace,Gregory N. Mace,J. Davy Kirkpatrick,Michael C. Cushing,Christopher R. Gelino,Ian S. McLean,Sarah E. Logsdon,Edward L. Wright,Michael F. Skrutskie,Charles A. Beichman,Peter Eisenhardt,Kristin R. Kulas +11 more
TL;DR: In this article, a wide separation (188''5) T8 subdwarf companion to the sdM1.5+WD binary Wolf 1130.9 is verified through common proper motion over a ~3 yr baseline.
Journal ArticleDOI
Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxies
Suzy Jones,Andrew Blain,Daniel Stern,Roberto J. Assef,Carrie Bridge,Peter Eisenhardt,Sara Petty,Jingwen Wu,Chao-Wei Tsai,Roc M. Cutri,Edward L. Wright,Lin Yan +11 more
TL;DR: In this article, the authors presented SCUBA-2 (Submillimetre Common-User Bolometer Array) 850μm submillimetres (submm) observations of the fields of 10 dusty, luminous galaxies at z ∼ 1.7-4.6, detected at 12 and/or 22 μm by the Wide-field Infrared Survey Explorer (WISE) all-sky survey, but faint or undetected at 3.4 and 4.6
Journal ArticleDOI
IDCS J1426.5+3508: Sunyaev-Zel'dovich Measurement of a Massive IR-selected Cluster at z=1.75
M. Brodwin,Anthony H. Gonzalez,S. A. Stanford,T. Plagge,Daniel P. Marrone,J. E. Carlstrom,A. Dey,Peter Eisenhardt,Cosimo Fedeli,D. Gettings,Buell T. Jannuzi,Marshall Joy,E. M. Leitch,C. Mancone,Gregory F. Snyder,D. Stern,Greg Zeimann +16 more
TL;DR: In this paper, a Sunyaev-Zel'dovich decrement is detected towards the IDCS J1426.5+3508 galaxy cluster, indicating a total mass of M200 = (4.3 +/- 1.1) x 10^{14} Msun in agreement with the approximate X-ray mass of 5 x 10−14 Msun.
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,Bradford P. Holden,Piero Rosati,Veronica Strazzullo,Nicole Homeier,Marc Postman,M. Franx,Alessandro Rettura,Holland C. Ford,G. D. Illingworth,Stefano Ettori,R. J. Bouwens,R. Demarco,Andre Martel,M. Clampin,George F. Hartig,Peter Eisenhardt,Acs Team +19 more
TL;DR: The color-magnitude relation for the RDCS J0910+5422 cluster of galaxies at redshift z = 1.106 has been determined in this paper, which shows that the blue early-type disk galaxies in this cluster likely represent the direct progenitors of the more evolved S0s that follow the same red sequence as ellipticals in other clusters.