Los Alamos National Laboratory / N. M. & Chudakov A. E. / /
Country
Germany / France / United States / Tibet / / /
Facility
George Mason University / University of New Hampshire / College Park / Louisiana State University / Columbia University / Max Planck Institute / New York University / Cabrillo College / Institute of Geophysics / University of Maryland / Massachusetts Institute of Technology / Purdue University / University of California / University of Wisconsin / For square / /
IndustryTerm
lower energy electrons / median energy / energy scale / triggered energy distribution / lower energy threshold / low-energy gamma rays / energy resolution / high-energy photons / imaging / energy response / lower energy primary photons / energy / low-energy background radiation / electronics / energy threshold / energy distribution / /
NaturalFeature
Fenton Hill / /
OperatingSystem
CYGNUS / /
Organization
Cabrillo College / University of California / University of New Hampshire / Durham / US Department of Energy / National Science Foundation / Max Planck Institute / Institute of Geophysics and Planetary Physics / Massachusetts Institute of Technology / University of Maryland / College Park / University of California / Irvine / Purdue University / Columbia University / New York / Stanford Linear Accelerator Center / New York University / New York / University of California / Santa Cruz / George Mason University / Louisiana State University / University of Wisconsin / Madison / American Astronomical Society / University of California / Riverside / Goddard Space Flight Center / /
Person
Ray Conf / Ray Astronomy / ESA SP / Stanford Linear / / /
Position
Corresponding author / /
ProvinceOrState
Wisconsin / Virginia / Alabama / Maryland / Indiana / Louisiana / New York / New Mexico / California / Massachusetts / New Hampshire / /
The Astrophysical Journal, 595:803–811, 2003 October 1 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. OBSERVATION OF TeV GAMMA RAYS FROM THE CRAB NEBULA WITH MILAGRO USING A NEW BACKG