All Tables

• Table 1: Summary of the RXTE observations used in this paper. PCA count rates represent count rates only from the upper layer of the PCU2 detector. HEXTE count rates are the count rates from one (of the two) clusters of detectors.
• Table 2: Best fit model parameters and inferred physical system parameters. Here C_F is the partial covering coefficient, F_3-100 the observed X-ray flux in the 3-100 keV band, F_0.1-100 the unabsorbed X-ray flux in the 0.1-100 keV band, both in 10^-11 erg cm^-2 s^-1 units. The distances for V405 Aur, V709 Cas, PQ Gem and V2400 Oph are assumed.
• Table 3: Comparison of different mass estimates. We present here masses obtained from broad band (3-100 keV) spectral fitting (Col. 2) and narrow band spectral fitting - our model (Cols. 3 and 4), work of Ramsay 2000 (Col. 5), work of Cropper et al. 1999 (Col. 6), and work of Ezucka & Ishida 1999 (Col. 7).