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Evan Scannapieco

Researcher at Arizona State University

Publications -  266
Citations -  9236

Evan Scannapieco is an academic researcher from Arizona State University. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 49, co-authored 263 publications receiving 8622 citations. Previous affiliations of Evan Scannapieco include Massachusetts Institute of Technology & University of California, Berkeley.

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LSST Science Book, Version 2.0

Paul A. Abell, +245 more
TL;DR: The Large Synoptic Survey Telescope (LSST) as discussed by the authors will have an effective aperture of 6.7 meters and an imaging camera with field of view of 9.6 degrees.
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The Type Ia Supernova Rate

TL;DR: In this article, the authors explore the idea that the Type Ia supernova (SN Ia) rate consists of two components: a prompt piece that is proportional to the star formation rate (SFR), and an extended piece that are proportional to total stellar mass.
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Quasar Feedback: The Missing Link in Structure Formation

TL;DR: In this paper, the authors consider the impact of quasar outflows on structure formation in the Lyα forest and show that quasar feedback fixes the turnover scale in the galaxy luminosity function (L*) as the nonlinear scale at the redshift of strong feedback.
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The detectability of the first stars and their cluster enrichment signatures

TL;DR: In this article, the first stars and their enrichment signatures in galaxy clusters were investigated and it was shown that the mean metallicity of outflows from Population III objects containing these stars is well above the critical transition metallity (Zcr ~ 10-4 Z☉) that marks the formation of normal stars.
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THERMONUCLEAR .Ia SUPERNOVAE FROM HELIUM SHELL DETONATIONS: EXPLOSION MODELS AND OBSERVABLES

TL;DR: In this article, the authors present hydrodynamic explosion models and observable outcomes of these He shell detonations for a range of initial core and envelope masses, and the peak UVOIR bolometric luminosities range by a factor of 10 (from 5×10 41 −5×10 42 erg s −1 ), and the R-band peak varies from MR,peak = −15 to −18.