Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-08-24
27th International Cosmic Ray Conference, Hamburg (Germany), 2001
Astronomy and Astrophysics
Astrophysics
4 pages, 6 Postscript figures; uses icrc.cls
Scientific paper
In atmospheric \v{C}erenkov technique $\gamma-$rays are detected against abundant background produced by hadronic showers. In order to improve signal to noise ratio of the experiment, it is necessary to reject a significant fraction of hadronic showers. The temporal and spectral differences, the lateral distributions and density fluctuations of \v{C}erenkov photons generated by $\gamma-$ray and hadron primaries are often used for this purpose. Here we study the differences in \v{C}erenkov photon density fluctuations at the observation level based on Monte Carlo simulations. Various types of density fluctuations like the short range (or local), medium range fluctuations and flatness parameter are studied. The estimated quality factors reflect the efficiencies with which the hadrons can be rejected from the data. It has been found that we can reject around 80% of proton showers while retaining about 70% of $\gamma-$ray showers in the data, based only on the differences in the flatness parameter. Density fluctuations particularly suited for wavefront sampling observations seem to be a good technique to improve the signal to noise ratio.
Bhat Narayan P.
Chitnis Varsha R.
No associations
LandOfFree
Gamma-Hadron Separation using Čerenkov Photon Density Fluctuations 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 Gamma-Hadron Separation using Čerenkov Photon Density Fluctuations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-Hadron Separation using Čerenkov Photon Density Fluctuations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-200084