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 T8.5 Brown Dwarf Member of the ξ Ursae Majoris System
Edward L. Wright,Mike Skrutskie,J. Davy Kirkpatrick,Christopher R. Gelino,Roger L. Griffith,Kenneth A. Marsh,Thomas H. Jarrett,Matthew J. Nelson,H. J. Borish,Gregory N. Mace,Amy Mainzer,Peter Eisenhardt,Ian S. McLean,John J. Tobin,Michael C. Cushing +14 more
TL;DR: The Wide-field Infrared Survey Explorer has revealed a T8.5 brown dwarf (WISE J111838.70+312537.9) that exhibits common proper motion with a solar-neighborhood (8 pc) quadruple star system as discussed by the authors.
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Radio Jet Feedback and Star Formation in Heavily Obscured, Hyperluminous Quasars at Redshifts ~ 0.5–3. I. ALMA Observations
C. J. Lonsdale,Mark Lacy,Amy Kimball,Amy Kimball,Andrew Blain,Mark Whittle,Belinda Jane Wilkes,D. Stern,James J. Condon,Minjin Kim,Minjin Kim,Roberto J. Assef,C. W. Tsai,Andreas Efstathiou,Suzy Jones,Peter Eisenhardt,Carrie Bridge,Jingwen Wu,Colin J. Lonsdale,K. Jones,Thomas H. Jarrett,R. Smith +21 more
TL;DR: In this paper, the Atacama Large Millimeter/submillimeter Array (ALMA) 870 μm (345 GHz) data for 49 high-redshift (0.47 < z < 2.85), luminous 11.7 < log (L_(bol/L_⊙) < 14.2) radio-powerful active galactic nuclei (AGNs), obtained to constrain cool dust emission from starbursts concurrent with highly obscured radiative-mode black hole (BH) accretion in massive galaxies that possess a small radio jet.
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Eddington-limited Accretion in z ∼ 2 WISE-selected Hot, Dust-obscured Galaxies
Jingwen Wu,Jingwen Wu,Hyunsung David Jun,Hyunsung David Jun,Roberto J. Assef,Chao-Wei Tsai,Edward L. Wright,Peter Eisenhardt,Andrew Blain,Daniel Stern,Tanio Díaz-Santos,Kelly D. Denney,Brian Hayden,Brian Hayden,Saul Perlmutter,Saul Perlmutter,Greg Aldering,Kyle Boone,Kyle Boone,Parker Fagrelius,Parker Fagrelius +20 more
TL;DR: Wu et al. as discussed by the authors measured the supermassive black hole masses of five z ∼ 2 Hot DOGs via broad Hα emission lines, using Keck/MOSFIRE and Gemini/FLAMINGOS-2.
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Spitzer Observations of the Prototypical Extremely Red Objects HR 10 and LBDS 53W091: Separating Dusty Starbursts from Old Elliptical Galaxies
TL;DR: In this paper, the Spitzer Space Telescope observations of the well-studied extremely red objects (EROs) HR 10 and LBDS 53W091 from 3.6 to 160 μm are presented.
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HUBBLE SPACE TELESCOPE MORPHOLOGIES OF z ∼ 2 DUST-OBSCURED GALAXIES. II. BUMP SOURCES
R. S. Bussmann,Arjun Dey,Jennifer M. Lotz,Lee Armus,Michael J. I. Brown,Vandana Desai,Peter Eisenhardt,J. L. Higdon,Sarah J.U. Higdon,Buell T. Jannuzi,E. Le Floc'h,Jason Melbourne,B. T. Soifer,Dan Weedman +13 more
TL;DR: In this paper, the spectral energy distribution (SED) of 22 ultra-luminous infrared galaxies (ULIRGs) at z ≈ 2 with extremely red R-[24] colors (called dust-obscured galaxies, or DOGs) was studied.