The mercedes-benz approach to γ-ray astronomy

Details The mercedes-benz approach to γ-ray astronomy The mercedes-benz approach to γ-ray astronomy

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988nimpa.264...74a&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 264, Issue 1, p. 74-80.

Physics

3

Scientific paper

The sensitivity requirements for ground-based γ-ray astronomy are reviewed in the light of the most reliable estimates of stellar fluxes above 100 GeV. Current data strongly favor the construction of detectors with the lowest energy thresholds. Since improvements in angular resolution are limited by shower fluctuations, better methods of rejecting hadronic showers must be found to reliably observe the known astrophysical sources. Several possible methods for reducing this hadronic background are discussed.

Affiliated with

Also associated with

No associations

Rating

The mercedes-benz approach to γ-ray astronomy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The mercedes-benz approach to γ-ray astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The mercedes-benz approach to γ-ray astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1227340