Very high energy gamma ray astrophysics
Our scientific goal is to discover and study by means of gamma-ray astronomy those regions of the universe where particles are accelerated to extreme energies. The atmospheric Cherenkov technique provides a unique and potentially sensitive window in the region of 10{sup 11} to approximately 10{sup 14} eV for this purpose. The Whipple Observatory Collaboration is currently engaged in the development of a Cherenkov camera which has the ultimate capability of distinguishing gamma-ray showers from the numerous cosmic-ray background showers by imaging the Cherenkov light from each shower. We have recently demonstrated the potential of the imaging technique with our 18 sigma detection of TeV photons from the Crab Nebula using a camera of 10 elements, pixel spacing 0.25 degrees. This detection represents a factor of 10 improvement in sensitivity compared to a non-imaging detector. The next step in the development of the detector is to obtain a second large reflector, similar to the present 10 meter instrument, for stereoscopic viewing of showers. This project, named GRANITE, is now approved by DOE. With GRANITE it should be possible to probe more deeply in space by a factor of 7, and to fully investigate the possibility of new physics which has been suggested by reports of anomalous radiation from Hercules X-1. 18 refs.
- Research Organization:
- Iowa State Univ. of Science and Technology, Ames, IA (USA)
- Sponsoring Organization:
- DOE/ER
- DOE Contract Number:
- AC02-80ER10774
- OSTI ID:
- 5076918
- Report Number(s):
- DOE/ER/10774-10; ON: DE90006645
- Country of Publication:
- United States
- Language:
- English
Similar Records
Observations of TeV photons at the Whipple Observatory
Observations of TeV photons at the Whipple Observatory
Very high energy gamma ray astrophysics: Progress report, May 1, 1987-February 1, 1988
Conference
·
Sun Dec 31 23:00:00 EST 1989
·
OSTI ID:6966224
Observations of TeV photons at the Whipple Observatory
Conference
·
Sun Dec 30 23:00:00 EST 1990
·
OSTI ID:10103967
Very high energy gamma ray astrophysics: Progress report, May 1, 1987-February 1, 1988
Technical Report
·
Sun Jan 31 23:00:00 EST 1988
·
OSTI ID:5605638
Related Subjects
440104 -- Radiation Instrumentation-- High Energy Physics Instrumentation
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
640101* -- Astrophysics & Cosmology-- Cosmic Radiation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ASTRONOMY
ASTROPHYSICS
BLACK HOLES
CHERENKOV COUNTERS
COSMIC RADIO SOURCES
CRAB NEBULA
DETECTION
DOCUMENT TYPES
GAMMA ASTRONOMY
GAMMA DETECTION
MEASURING INSTRUMENTS
NEBULAE
PROGRESS REPORT
RADIATION DETECTION
RADIATION DETECTORS
RESEARCH PROGRAMS
SUPERNOVA REMNANTS
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
640101* -- Astrophysics & Cosmology-- Cosmic Radiation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ASTRONOMY
ASTROPHYSICS
BLACK HOLES
CHERENKOV COUNTERS
COSMIC RADIO SOURCES
CRAB NEBULA
DETECTION
DOCUMENT TYPES
GAMMA ASTRONOMY
GAMMA DETECTION
MEASURING INSTRUMENTS
NEBULAE
PROGRESS REPORT
RADIATION DETECTION
RADIATION DETECTORS
RESEARCH PROGRAMS
SUPERNOVA REMNANTS