LINKS
Introduction to Gamma Ray Astronomy
Observer Home Page (restricted access)
Whipple Software
MajorCool E-mail List Manager
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Data Archiving using DVD-RAM with Linux
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GRANITE III CAMERA - FINAL
10 Meter Atmospheric Cherenkov Telescope
The Purdue HEAp group is engaged in experiments in ground-based Very
High Energy (VHE) Gamma Ray astrophysics utilizing the 10 meter atmospheric Cherenkov telescope (shown
above) at the Whipple Observatory
in Arizona.
The objective of these experiments is the search for and study of
astrophysical sources of gamma-rays with energies of
100 GeV to 10 TeV, an energy region well beyond the range
of current orbiting gamma-ray detectors. For more detail,
click here.
Recently the group has been monitoring
time variable signals from Markarian 421, a B L Lac galaxy some 500
million light-years distant, which has a superluminal jet of
relativistic particles beamed towards www. Present models suggest
that the enormous energy output of this galaxy derives from a rotating
supermassive black hole in its nucleus. In addition, another B L Lac galaxy,
Markarian 501, has been detected in the Gev domain.
The VHE Gamma-ray air shower simulations by DePauw-Purdue can be seen in
the following links:
KASCADE  
ENERGY  
RAYTRACE  
CFD
Currently the Whipple collaboration is in the process of carrying out an
upgrade of the present camera from 151 1" pixel elements to a 541
element camera consisting of both 1/2" and 1" pixel elements. The Purdue
HEAp group is responsible for the testing and calibration of the PMTs which will comprise the new camera.
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