Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.
Science Signaling - Call for Papers

Site Tools

  • AAAS
  • Subscribe
  • Feedback

Site Search

Search Advanced

Science 5 January 2007:
Vol. 315. no. 5808, pp. 70 - 72
DOI: 10.1126/science.1136395

Perspective

The Very-High-Energy Gamma-Ray Sky

Felix Aharonian1,2

Over the past few years, very-high-energy gamma-ray astronomy has emerged as a truly observational discipline, with many detected sources representing different galactic and extragalactic source populations—supernova remnants, pulsar wind nebulae, giant molecular clouds, star formation regions, compact binary systems, and active galactic nuclei. It is expected that observations with the next generation of stereoscopic arrays of imaging atmospheric Cherenkov telescopes over a very broad energy range from 1010 to 1015 electron volts will dramatically increase the number of very-high-energy gamma-ray sources, thus having a huge impact on the development of astrophysics, cosmology, and particle astrophysics.

1 Dublin Institute for Advanced Studies, Dublin, Ireland.
2 Max Planck Institut fur Kernphysik, Heidelberg, Germany.

E-mail: Felix.Aharonian{at}mpi-hd.mpg.de

Read the Full Text






ADVERTISEMENT
Click Me!

ADVERTISEMENT
Click Me!

To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)