S
Sean T. Scully
Researcher at James Madison University
Publications - 50
Citations - 1957
Sean T. Scully is an academic researcher from James Madison University. The author has contributed to research in topics: Redshift & Intergalactic travel. The author has an hindex of 26, co-authored 49 publications receiving 1864 citations. Previous affiliations of Sean T. Scully include Valparaiso University & Goddard Space Flight Center.
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Intergalactic Photon Spectra from the Far-IR to the UV Lyman Limit for 0 < z < 6 and the Optical Depth of the Universe to High-Energy Gamma Rays
TL;DR: In this article, the optical depth of the universe to gamma-rays; tau; and tau coefficient were incorrectly calculated for various redshifts for the baseline model (upper row) and fast evolution (lower row) for individual redshift.
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Light-Element Evolution and Cosmic-Ray Energetics
TL;DR: In this paper, the authors investigate the viability of evolutionary models for the light elements Li, Be, and B (LiBeB) and find that models in which the cosmic rays are accelerated mainly out of the average interstellar medium which is increasingly metal-poor at early times significantly underpredict the measured Be abundance of the early Galaxy.
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An empirical determination of the intergalactic background light from uv to fir wavelengths using fir deep galaxy surveys and the gamma-ray opacity of the universe
TL;DR: In this article, Stecker et al. determined the intergalactic background light (IBL) as a function of redshift in the far ultraviolet to near infrared range, based purely on data from deep galaxy surveys.
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Searching for traces of Planck-scale physics with high energy neutrinos
TL;DR: In this article, the authors consider a class of non-renormalizable, Lorentz invariance violating operators that arise in an effective field theory (EFT) description of neutrino sector inspired by Planck-scale physics and quantum gravity models.
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The Effects of an Early Galactic Wind on the Evolution of D,3He, and Z
TL;DR: In this article, the role of an early episode of massive star formation that would induce a strong destruction of D and a galactic wind was examined and the ability of these models to match the observed local properties of the solar neighborhood such as the gas mass fraction, oxygen abundance, the age-metallicity relation, and the present-day mass function.