All Tables

• Table 1: Models of the nova spatial distribution in the Galaxy used for the Monte Carlo simulations (Jean et al. 2000).
• Table 2: The probability that a novae is detectable with BAT, for each of four energy bins. Results are for the spatial distribution of model 1 in Table 1. Other distribution models give very similar results (see text for details).
• Table 3: The 24 classical novae examined in the search for the prompt gamma-ray emission.
• Table 4: Summary of the results obtained from BAT data for 24 Classical novae.