All Tables

Table 1: The comparison of the $\beta$ -model fitting results for the galaxy cluster CL0016+16.
Table 2: The spectral-fit results of the temperature profile with frozen and free abundances for all EPIC cameras.
Table 3: The spectral fits results in the chosen regions, with free abundances. Three EPIC cameras were used.
Table 4: The $\beta$ -model fitting results in different directions.
Table 5: The results of CL0016+16 mass analysis using different temperature profiles and cluster parameters.
Table 6: The best-fitting results of the 2D $\beta$ -model, from the XMM-Newton and Chandra data