Understanding gamma-ray burst emission physics with multiwavelength data

该奖项是根据2009年美国复苏和再投资法案（公法111-5）资助的。这是一个计划，以执行伽马射线暴（GRB）的多波长研究：1。系统地分析伽玛暴余辉数据，明确识别出具有明显物理来源的辐射成分; 2.使用复杂的外部前向激波模型对宽带、多分量余辉进行详细建模; 3.分析Swift/BAT和Fermi/GBM收集的γ暴瞬发数据，并考察各种经验关联式的有效性;模拟伽玛暴的宽带瞬发辐射。 数据将来自斯威夫特和费米太空任务，以及地面上的HESS和VERITAS。

This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).This is a program to perform a multi-wavelength study of Gamma Ray Bursts (GRBs) to: 1. Systematically analyze GRB afterglow data, and clearly identify emission components that have distinct physical origins; 2. Perform detailed modeling of broadband, multi-component afterglows using a sophisticated external forward shock model; 3. Analyze the GRB prompt emission data collected by Swift/BAT and Fermi/GBM, and investigate the validity of various empirical correlations; and 4. Model the broad band prompt emission of GRBs. Data will come from the Swift and Fermi space missions, and from HESS and VERITAS on the ground.