Los Alamos National Laboratory / USA 8 Columbia Astrophysics Laboratory / Denmark 6 Lawrence Livermore National Laboratory / Ge / Wilson / Pearson / USA 4 Space Sciences Laboratory / USA 9 Jet Propulsion Laboratory / /
Country
United States / Canada / /
Facility
Columbia University / National Space Institute / Technical University of Denmark / NC State University / California Institute of Technology / University of California / Observatory Obs / McGill University / /
IndustryTerm
steady-state solutions / high-resolution imaging / upper energy range / energy bands / radial / low energy band / energy range / high energy particles / absorbed power law / measured power-law index / detector chips / average photon energy / broken power law / energy resolution / absorbed power-law model / imaging / energy / break energy / lower energy spectral channels / energy band / low-energy highresolution / steppar tool / high energy electrons / lowest energy band / average energy / detector chip / arestore tool / obs tool / synchrotron energy losses / double power-law model / power-law functions / chandra repro tool / power law / power-law model / low energy data / energy distribution / power-law index / energy ranges / reprocessed using the chandra repro tool / /
MusicGroup
X-RAY / /
Organization
Technical University of Denmark / California Institute of Technology / Columbia University / Physics Department / University of California / Berkeley / National Space Institute / Department of Physics / Cahill Center for Astronomy and Astrophysics / NC State University / Raleigh / McGill University / Montreal / Goddard Space Flight Center / /
Draft version August 4, 2014 Preprint typeset using LATEX style emulateapj v[removed]arXiv:1408.0174v1 [astro-ph.HE] 1 Aug[removed]HIGH-ENERGY X-RAY IMAGING OF THE PULSAR WIND NEBULA MSH 15−52: CONSTRAINTS ON