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2.3.4 Source Count Rates

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.



  
Table 4: X-ray Count rates (counts s-1) for different instruments
  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
Notes: v - variable source, the count rate for A2256 is determined from the net emission within a 6' radius.


next up previous contents
Next: 2.4 Background Up: 2.3 Effective Area Previous: 2.3.3 Long-term stability
rsdc@cfa.harvard.edu
1999-05-25