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Phil A. Evans (2) ((1) UT Austin

Identifiers

  • name variant Phil A. Evans (2) ((1) UT Austin 0.60 · backfill

Papers (1)

  1. The Dust Scattering Model Can Not Explain The Shallow X-ray Decay in GRB Afterglows astro-ph · 2008 · author #5

Mentions

  • 0806.3541 #5 · backfill · confidence 0.70 Phil A. Evans (2) ((1) UT Austin

Frequent Coauthors