For #1, an examination of light curves and plots of the KS test show that there are many intervals and obis when no activity is seen. #2 is quite different, being more steady (less ``sparking'' or ``flickering''). For the first two, the average count rate drops quickly as the length of the time bin is increased. As mentioned previously, #3 is relatively constant.
| HS #1 | #2 | #3 | |
| First known occurrence | 8Jul95/rh800694 | mid-Mar95 | 27Jan97 |
| Largest known c/s (1 s bins) | 57(rh300399) | much less than #1 | ----- |
| Largest known <c/s> for a seq: | 0.76 (17.2 ks) | 0.0177(28 ks) | 0.039(2.5 ksec) |
| (rh202596) | |||
| Incidence of Detection | 120 out of 240 seqs; | 7/240 | almost all |
| (Jul-Sep 1995) |