Table 2
Three σ c.l. upper limits on the pulsed fraction of IGR J18410-0535 (see notes below the table).
| XMM-Newton (0.3–12 keV) | |||
|
|
|||
| Time interval | Instrument (time resolution) | ||
|
|
|||
| PN (73.4 ms) | MOS1 (0.3 s) | MOS2 (1.75 ms) | |
|
|
|||
| A+B+C+D+E+F+G+H+I+J+K+L+M+N+O | 6–10% (0.02–6.8 Hz) | 10–20% (0.01–1.6 Hz) | 15–30% (0.02–286 Hz) |
| C+D+E+F+G+H | 10–30% (0.04–6.8 Hz) | 10–30% (0.01–1.6 Hz) | 10–30% (0.03–286 Hz) |
| C+D | 30–50% (0.05–6.8 Hz) | 50–70% (0.1–1.6 Hz) | 60–80% (0.06–286 Hz) |
| E | 20–35% (0.05–6.8 Hz) | 20–35% (0.03–1.6 Hz) | 20–70% (0.1–286 Hz) |
| F+G+H | 15–20% (0.08–6.8 Hz) | 20–30% (0.02–1.6 Hz) | 20–30% (0.05–286 Hz) |
| J+K+L | 10–20% (0.02-6.8 Hz) | 20–40% (0.01–1.6 Hz) | 35–60% (0.02–286 Hz) |
| M+N | 40–60% (0.02–6.8 Hz) | 75–100% (0.02–1.6 Hz) | 80–100% (0.02–286 Hz) |
|
|
|||
| ASCA (0.7–10 keV) | |||
|
|
|||
| GIS (0.5 s) | |||
|
|
|||
| Obs.1+Obs.2 | 30–45% (0.01–1 Hz) | ||
Notes. The three σ upper limits on the pulsed fraction of IGR J18410-0535 are determined for the three Epic cameras in the different time intervals reported in Table 1. The results of a similar analysis carried out on the ASCA data are also reported (see Sect. 3.1 for the discussion of the ASCA data analysis).
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