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Table 1
Effective exposure time of each XMM-Newton -EPIC and Chandra-ACIS observation.
| XMM-Newton | Centre coordinates | MOS1 effective | MOS2 effective | PN effective |
| obs. IDs | exposure time (ks) | exposure time (ks) | exposure time (ks) | |
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| 0112230601 | 16h15m46.01s –06°09′00.0″ | 8.8 (56.2%) | 9.8 (63.5%) | 5.7 (56.2%) |
| 0112230701 | 16h16m48.00s –06°09′00.0″ | 11.8 (42.5%) | 12.1 (43.4%) | 6.1 (29.9%) |
| 0112230801 | 16h15m46.01s –05°51′00.0″ | 16.1 (57.5%) | 14.6 (52.2%) | 10.2 (49.0%) |
| 0112230901 | 16h14m34.01s –06°09′00.0″ | 7.4 (27.5%) | 6.9 (25.5%) | 3.3 (16.7%) |
| 01122301001 | 16h15m46.01s –06°27′00.0″ | 19.5 (69.3%) | 16.5 (58.8%) | 15.4 (72.4%) |
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| Chandra obs ID | Centre coordinates | ACIS effective exposure time (ks) | ||
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| 01653 | 16h15m45.77s –06° 08′55.0″ | 65.2 (91.7%) | ||
Notes. In brackets: fraction of the useful exposure time after solar-flare “cleaning”.
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