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Table 5.5
shows measured HRI count rates for a sample of sources and
compares these rates to that of the PSPC and the Einstein
Observatory HRI and IPC.
| Object | ROSAT | Einstein | ROSAT | Einstein |
| | HRI | HRI | PSPC | IPC |
| HZ 43 | 12.0 | 3.6 | 100 | 3.8 |
v | AR Lac | 0.65 | 0.69 | 7.4 | 1.3 |
v | Cyg X-2 | 72 | 27.8 | 180 | NA |
v | LMC X-1 | 3.8 | 1.3 | 10 | 10.55 |
v | LMC X-3 | 2.6 | 2.7 | NA | NA |
| Cas A | 17 | 6.3 | 57 | 61 |
| Tycho | 10.2 | 3.4 | NA | 22.3 |
| Kepler | 5.4 | 1.7 | NA | 7.3 |
| E 0102.2-72.2 (SMC SNR) | 0.96 | 0.25 | NA | 0.79 |
| N132D | 3.6 | 1.1 | 10.6 | 4.0 |
a | A 2256 | 0.62 | NA | 1.7 | 0.34 |
v: variable source |
a: the count rate for A 2256 is determined from
the net emission within a 6' radius |
Table 5.5: Comparison of X-ray count rates
(counts/s) between the HRI/PSPC detectors of ROSAT
and the HRI/IPC detectors of Einstein
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