Table 4 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 | ||
HZ43 | 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 | |
E0102.2-72.2 | 0.96 | 0.25 | NA | 0.79 | |
(SMC SNR) | |||||
N132D | 4.5 | 1.1 | 10.6 | 4.0 | |
A2256 | 0.62 | NA | 1.7 | 0.34 |