Observations of TeV photons at the Whipple Observatory
Conference
·
OSTI ID:6966224
- Iowa State Univ. of Science and Technology, Ames, IA (United States)
- Michigan Univ., Ann Arbor, MI (United States)
- Saint Patrick's Coll., Maynooth (Ireland)
- Harvard-Smithsonian Center for Astrophysics, Amado, AZ (United States)
The Whipple Observatory 10 m gamma-ray telescope has been used to search for TeV gamma-ray emission from a number of objects. This paper reports observations of six galactic and three extragalactic objectsusing the Cherenkov image technique. With the introduction of a high-resolution camera (1/4[degree] pixel) in 1988, the Crab Nebula was detected at a significance level of 20 [omega], in 30 hours of on-source observation. Upper limits at a fraction of the Crab flux are set for most of the other objects, based on the absence of any significant dc excess or periodic effect when an a priori Monte Carlo determined imaging selection criterion (the azwidth cut'') is employed. There are weak indications that one source, Hercules X-1, may be an episodic emitter. The Whipple detection system will be improved shortly with the addition of a second reflector 11 m in diameter (GRANITE) for stereoscopic viewing of showers. The combination of the two-reflector system should have a signal-to-noise advantage of 10[sup 3] over a simple nonimaging Cherenkov receiver.
- Research Organization:
- Iowa State Univ. of Science and Technology, Ames, IA (United States)
- Sponsoring Organization:
- DOE; USDOE, Washington, DC (United States)
- DOE Contract Number:
- AC02-80ER10774
- OSTI ID:
- 6966224
- Report Number(s):
- CONF-9010289-5; ON: DE93003720
- 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. [Her X-1; Cyg X-3; PSR 0355+54; M1; NGC 1952; 1E 2259+586; 4U 0115+63; M87; 3C 273; 3C 279]
Very high energy gamma ray astrophysics
Conference
·
Sun Dec 30 23:00:00 EST 1990
·
OSTI ID:10103967
Observations of TeV photons at the Whipple Observatory. [Her X-1; Cyg X-3; PSR 0355+54; M1; NGC 1952; 1E 2259+586; 4U 0115+63; M87; 3C 273; 3C 279]
Conference
·
Thu Apr 04 23:00:00 EST 1991
· AIP Conference Proceedings (American Institute of Physics); (United States)
·
OSTI ID:5667209
Very high energy gamma ray astrophysics
Technical Report
·
Wed Jan 31 23:00:00 EST 1990
·
OSTI ID:5076918
Related Subjects
440104 -- Radiation Instrumentation-- High Energy Physics Instrumentation
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
661300* -- Other Aspects of Physical Science-- (1992-)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ASTRONOMY
CALCULATION METHODS
COSMIC GAMMA SOURCES
COSMIC RADIO SOURCES
COSMIC RAY SOURCES
CRAB NEBULA
DETECTION
FREQUENCY DEPENDENCE
GAMMA ASTRONOMY
GAMMA DETECTION
MONTE CARLO METHOD
NEBULAE
RADIATION DETECTION
SUPERNOVA REMNANTS
TELESCOPES
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
661300* -- Other Aspects of Physical Science-- (1992-)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ASTRONOMY
CALCULATION METHODS
COSMIC GAMMA SOURCES
COSMIC RADIO SOURCES
COSMIC RAY SOURCES
CRAB NEBULA
DETECTION
FREQUENCY DEPENDENCE
GAMMA ASTRONOMY
GAMMA DETECTION
MONTE CARLO METHOD
NEBULAE
RADIATION DETECTION
SUPERNOVA REMNANTS
TELESCOPES