E
Eliot Quataert
Researcher at University of California, Berkeley
Publications - 242
Citations - 15951
Eliot Quataert is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Galaxy & Accretion (astrophysics). The author has an hindex of 66, co-authored 242 publications receiving 14271 citations. Previous affiliations of Eliot Quataert include University of California & UCB.
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Journal ArticleDOI
Synthetic Gaia surveys from the FIRE cosmological simulations of Milky Way-mass galaxies.
Robyn E. Sanderson,Andrew Wetzel,Sarah Loebman,Sanjib Sharma,Philip F. Hopkins,Shea Garrison-Kimmel,Claude André Faucher-Giguère,Dušan Kereš,Eliot Quataert +8 more
TL;DR: Ananke as discussed by the authors is a framework for generating synthetic phase-space surveys from high-resolution baryonic simulations, and use it to generate a suite of synthetic surveys resembling Gaia DR2 in data structure, magnitude limits, and observational errors.
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Variations in the spectral slope of Sgr A* during a NIR flare
Stefan Gillessen,Frank Eisenhauer,Eliot Quataert,Reinhard Genzel,Thibaut Paumard,Sascha Trippe,Thomas Ott,Roberto Abuter,Andreas Eckart,P. O. Lagage,Matt Lehnert,Linda J. Tacconi,Fabrice Martins +12 more
TL;DR: In this paper, a bright flare of Sgr A* in the near infrared with the adaptive optics assisted integral field spectrometer SINFONI was observed and the observed spectrum is featureless and can be described by a power law.
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Setting the Stage for Circumstellar Interaction in Core-Collapse Supernovae II: Wave-Driven Mass Loss in Supernova Progenitors
J. Shiode,Eliot Quataert +1 more
TL;DR: In this article, the authors explore the internal conditions of SN progenitors using the MESA 1-D stellar evolution code, in search of those most susceptible to wave-driven mass loss.
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Nonthermal THz to TeV Emission from Stellar Wind Shocks in the Galactic Center
Eliot Quataert,Abraham Loeb +1 more
TL;DR: In this article, the relativistic electrons inverse Compton scatter the ambient ultraviolet and far-infrared radiation field, producing high-energy γ-rays with a roughly constant luminosity from ~GeV to ~10 TeV.
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On the Validity of the Classical Apsidal Motion Formula for Tidal Distortion
TL;DR: In this paper, the authors check the validity of the widely used classical apsidal motion formula as a function of orbital parameters, stellar structure, and stellar rotation rate by comparing dynamical calculations of the periastron advance with the static tidal formula.