Table 1.
Summary of the extended source simulations in the ROSAT-like images.
| Input flux (0.5 − 2.0 keV) (erg s−1 cm−2) | Input core radius |
|||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| 0.75′ | 1.50′ | 2.25′ | 3.00′ | 3.75′ | 4.50′ | 5.25′ | 6.00′ | 12.00′ | 24.00′ | |
| 1 × 10−12 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 25 | 100 |
| 3 × 10−12 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 25 | 100 |
| 5 × 10−12 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 25 | 100 |
| 1 × 10−11 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 25 | 100 |
| 5 × 10−11 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 20 | 25 | 100 |
Notes. The column values indicate the number of simulated images for a given β value. For each set of parameters ( β, rc, and flux within rc), 100 clusters are simulated. For example, a value of 20 in the table means that there are 5 clusters in one simulated image for a given set of parameters. Simulations were performed for an exposure time of 450 s with a background level of 0.08 cnts pixel−1, and four β values (0.40, 0.55, 0.66, and 0.70).
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