Award Abstract #0820875
MRI: Development of the HAWC-256 Wide-Field Gamma Ray Detector

NSF Org:	PHY Division of Physics
Initial Amendment Date:	August 21, 2008
Latest Amendment Date:	August 21, 2008
Award Number:	0820875
Award Instrument:	Standard Grant
Program Manager:	James J. Whitmore PHY Division of Physics MPS Directorate for Mathematical & Physical Sciences
Start Date:	September 1, 2008
Expires:	August 31, 2011 (Estimated)
Awarded Amount to Date:	$605000
Investigator(s):	Jordan Goodman goodman@umdgrb.umd.edu (Principal Investigator) Andrew Smith (Co-Principal Investigator)
Sponsor:	University of Maryland College Park 3112 LEE BLDG COLLEGE PARK, MD 20742 301/405-6269
NSF Program(s):	MAJOR RESEARCH INSTRUMENTATION
Field Application(s):	0000099 Other Applications NEC
Program Reference Code(s):	OTHR, 7483, 1189, 0000
Program Element Code(s):	1189

ABSTRACT

High energy gamma rays probe the most extreme astrophysical environments including those that produce the highest energy cosmic-ray particles. Most of the discoveries in the TeV energy range have been made by imaging atmospheric Cherenkov telescopes (IACTs) which have a few milli-steradian field of view and ~10% duty cycle. However, the Milagro observatory has demonstrated that a detector with a wide field of view and nearly 100% duty cycle can discover new sources of TeV gamma rays at energies between 10 and 100 TeV, and map the diffuse emission from the plane of our Galaxy. The HAWC (High Altitude Water Cherenkov) observatory builds on the experience and technology of Milagro to make a second-generation high-sensitivity detector that would be capable of continuously surveying the TeV sky for steady and transient sources from 100 GeV to 100 TeV.

This MRI award is to develop the HAWC electronics and instrumentation by building a core array at high altitude. This instrument will be developed by a collaboration from the US and Mexico, led by the US team that built Milagro and pioneered the development of the water Cherenkov technique for gamma-ray astronomy. It will be located near Sierra Negra, Mexico, at an altitude of 4100m near existing infrastructure and collaborating universities and will allow the development of Cherenkov detectors and electronics at high altitude as a prelude to eventually building the entire HAWC detector.

Beyond astrophysics, this will establish a preeminent international scientific collaboration with particle physicists and astrophysicists in Mexico. The collaboration will utilize this unique opportunity to reach out to Hispanics as well as maintain the Milagro tradition of providing strong scientific and educational opportunities for undergraduate students, graduate students, and post-doctoral fellows.

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