Abstract
We present a Monte Carlo analysis of the recently introduced variability
indices $\tau$ (Tompkins 1999) and $I$ (Zhang et al. 2000 & Torres et al. 2001)
for $\gamma$-ray sources. We explore different variability criteria and prove
that these two indices, despite the very different approaches used to compute
them, are statistically correlated (5 to 7$\sigma$). This conclusion is
maintained also for the subset of AGNs and high latitude ($|b|>10$ deg)
sources, whereas the correlation is lowered for the low latitude ones, where
the influence of the diffuse galactic emission background is strong.
Originalsprog | Engelsk |
---|---|
Tidsskrift | Astronomische Nachrichten |
Vol/bind | 322 |
Udgave nummer | 4 |
Sider (fra-til) | 223-227 |
Antal sider | 4 |
ISSN | 0004-6337 |
DOI | |
Status | Udgivet - 30 okt. 2001 |