![Loading...](https://link.springer.com/static/c4a417b97a76cc2980e3c25e2271af3129e08bbe/images/pdf-preview/spacer.gif)
-
Article
Development of the atmospheric Cherenkov imaging technique
Following a brief history of the atmospheric Cherenkov imaging technique and a summary of the current status of the field, we describe some of the potential developments of the method over the next few years. ...
-
Article
Extremely rapid bursts of TeV photons from the active galaxy Markarian 421
DISCRETE astronomical sources of photons in the TeV energy range are believed to be associated with regions in the relativistic outflow of particles and radiation from compact objects, such as neutron stars an...
-
Article
Instrumentation for very high energy gamma-ray astronomy
Considerable progress has been made in the last half-decade in the field of very high energy (VHE) gamma-ray astronomy (photons with energies between 1011 and 1013 eV). The high background level due to the isotro...
-
Article
Detection of TeV photons from the active galaxy Markarian 421
PHOTONS of TeV energy have been observed from a few sources in our Galaxy, notably the Crab Nebula1. We report here the detection of such photons from an extragalactic source, the giant elliptical galaxy Markaria...
-
Article
A high resolution imaging detector for TeV gamma-ray astronomy
Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter opti...
-
Chapter
Observation of TeV Gamma-rays from the Crab Nebula
The Whipple Observatory 10 m Reflector operating as a 37-pixel camera has been used to observe the Crab Nebula in TeV gamma rays. Using gamma-ray image selection a detection is reported at the 9.0 sigma level;...
-
Chapter
Search for Pulsed TeV Emission from PSR0531+21
The Crab pulsar (PSR0531+21) has been observed with the Whipple Observatory 10 m Reflector in imaging mode for ~102h. A suggestion of a broad light curve has been found, but with a low statistical significance...
-
Chapter
Observation of TeV Gamma-rays from the Crab Nebula and PSR 0531
The Whipple Observatory 10 m Reflector operating as a 37-pixel camera has been used to observe the Crab Nebula in TeV gamma rays. Using gamma-ray image selection a detection is reported at the 9.0 sigma level;...
-
Chapter
Pulsed TeV Gamma Rays from 4u0115+63
The transient X-ray binary pulsar, 4U0115+63, has been observed for 37 hours by the Whipple Observatory Cherenkov imaging camera between September 1985 and January 1986. These observations were grouped into ni...
-
Chapter
TeV Observations of Her X-l at the Whipple Observatory: 1984–1985
Her X-l has been observed for 73 hours with the Whipple Observatory Cerenkov imaging camera on the 10m reflector between April 1984 and June 1985. Seven distinct episodes of emission were seen, ranging in dura...
-
Chapter
Search for TeV Gamma rays from the Galactic Plane near Cygnus X-3
The null results of a search for gamma-ray emission at TeV energies from the galactic plane near Cygnus X-3 are reported.
-
Chapter
Search for a 12.59 ms. Pulsar in Cygnus X-3 at E > 400 GeV
A high energy (E > 400 GeV) gamma ray database on Cygnus X-3 covering the observational interval 1983–1985 has been examined for possible evidence of a 12.5908 ms. pulsar, as recently reported by Chadwick et a...