Add to ORKGThe Haverah Park 50 m water-Cerenkov array has been used to examine a number of periodic sources for ultra high energy gamma-ray emission above 10 to the 15th power eV. The data, recorded between 1 Jan. 1979 and 31 Dec. 1984, feature a modest angular resolution of approx 3 deg with millisecond arrival time resolution post 1982. The sources investigated include the Crab pulsar, Her X-1, Au0115 + 63 and Geminga. All objects have been detected by workers in the TeV region, with varying degrees of confidence
Invited talk at the XXIV Physics in Collisions Conference (PIC04), Boston, USA, June 2004, 10 pages,...
The arrival directions of the gamma-quanta with energies of about 10 to 15th power eV which were reg...
Data on Crab pulsar from atmospheric Cerenkov array at Ooty have shown emission of TeV gamma rays in...
It is now more than 20 years since the first ground based gamma ray experiments involving atmospheri...
Flux limits in the range 10 to the minus 13th power-10 to the minus 12 power/sq cm/s have been obtai...
The detection of very high energy gamma ray sources has been reported in the last few years by means...
Data from the University of Adelaide air shower array at Buckland Park taken over a three year perio...
Observations of the Crab pulsar using the atmospheric Cerenkov technique were conducted for 22 hours...
Considerable interest has developed in the search for local sources of superhigh-energy gamma-rays. ...
This thesis describes the observation of a number of astronomical objects using the University of Du...
The discovery of cosmic rays with energies greater than 1014e V has posed a question that has not, a...
The hypothesis that there exists an excess of showers from the Galactic plane on the level 1 to 2% a...
Radio pulsars have concentrated on long observations of the Crab pulsar and showed that it emits sho...
The design and operation of a 32 x 1 10 to the 15th power sq m array of scintillation detectors for ...
A search was conducted for TeV gamma-rays emitted from the direction of the ultra-high-energy cosmic...
Invited talk at the XXIV Physics in Collisions Conference (PIC04), Boston, USA, June 2004, 10 pages,...
The arrival directions of the gamma-quanta with energies of about 10 to 15th power eV which were reg...
Data on Crab pulsar from atmospheric Cerenkov array at Ooty have shown emission of TeV gamma rays in...
It is now more than 20 years since the first ground based gamma ray experiments involving atmospheri...
Flux limits in the range 10 to the minus 13th power-10 to the minus 12 power/sq cm/s have been obtai...
The detection of very high energy gamma ray sources has been reported in the last few years by means...
Data from the University of Adelaide air shower array at Buckland Park taken over a three year perio...
Observations of the Crab pulsar using the atmospheric Cerenkov technique were conducted for 22 hours...
Considerable interest has developed in the search for local sources of superhigh-energy gamma-rays. ...
This thesis describes the observation of a number of astronomical objects using the University of Du...
The discovery of cosmic rays with energies greater than 1014e V has posed a question that has not, a...
The hypothesis that there exists an excess of showers from the Galactic plane on the level 1 to 2% a...
Radio pulsars have concentrated on long observations of the Crab pulsar and showed that it emits sho...
The design and operation of a 32 x 1 10 to the 15th power sq m array of scintillation detectors for ...
A search was conducted for TeV gamma-rays emitted from the direction of the ultra-high-energy cosmic...
Invited talk at the XXIV Physics in Collisions Conference (PIC04), Boston, USA, June 2004, 10 pages,...
The arrival directions of the gamma-quanta with energies of about 10 to 15th power eV which were reg...
Data on Crab pulsar from atmospheric Cerenkov array at Ooty have shown emission of TeV gamma rays in...