Gamma Ray Astronomy

At

Purdue University

LINKS


Introduction to Gamma Ray Astronomy

Observer Home Page (restricted access)

Whipple Software

MajorCool E-mail List Manager

Whipple Nightly Archives

Whipple List Archives

Data Archiving using DVD-RAM with Linux

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.


For more information on

Markarian 421:
Multiwavelength Observations of Markarian 421 During a Tev X-Ray Flare
An Upper Limit to the Infrared Background
from Observations of Tev Gamma Rays
Outburst of TeV Photons from Markarian 421
Markarian 501:
Detection of Gamma Rays with E>300 GeV From Markarian 501





Contributions to the 4th Compton Science Symposium

April 27 - 30 1997, Williamsburg, VA

VHE AND UHE Gamma Ray Astronomy Invited Review Talk
Constraints on Cosmic-Ray Origin from TeV Gamma-Ray Observations
of Supernova Remnants
Whipple Observations of BL Lac Objects at E > 300 GeV
Very High Energy Observations of PSR B1951+32
The Spectrum of TeV Gamma-Rays from the Crab Nebula
Multiwavelength observations of Markarian 421
The energy spectrum of Markarian 421 between 300 GeV - 5 TeV
Stereo Observations with the Whipple 10m/11m detector
VERITAS: the Very Energetic Radiation Imaging Telescope Array System




23 June 1999