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Table 5
Measured cts/s during the occultation phases of the ten selected sources in this work.
| Source | 17−40 keV | 40−150 keV |
| cts/s | cts/s | |
|
|
||
| LMC X-4 | 0.9(1) | 0.7(1) |
| Cen X-3 | 0.27(8) | − |
| 4U 1700-377 | 1.31(8) | 0.50(6) |
| 4U 1538-522 | − | − |
| SMC X-1 | 0.48(16) | − |
| SAX J1802.7-2017 | 0.35(7) | − |
| XTE J1855-026 | − | − |
| Vela X-1 | 1.02(7) | 0.15(6) |
| EXO 1722-363 | − | − |
| OAO 1657-415 | 0.60(7) | 0.23(7) |
Notes. Note that 0.2 cts/s (0.1 cts/s) in the 17−40 keV (40-150 keV) energy band in ISGRI correspond to roughly 1 mCrab. We indicate in brackets the uncertainties at 90% c.l. on the last digits of each reported value.
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