Table 3
HMXBs in the LMC: Variability between observations.
| No. | 700016 | 700161 | 700156 | 700179 | 700184 | 700185 |
|---|---|---|---|---|---|---|
| 2019–09–15 | 2019–10–18 | 2019–10–10 | 2019–11–22 | 2019–11–23 | 2019–11–25 | |
| 71 | <4.6×10−3 | <5.2×10−3 | <2.0×10−3 | |||
| 5 | – | – | <5.8×10−3 | 5.40 ± 1.28 × 10−3 | 6.79 ± 0.93 × 10−3 | – |
| 33 | – | – | <2.9×10−3 | <6.6×10−3 | <1.6×10−3 | – |
| 35 | – | – | 1.14 ± 0.15 × 10−2 | 1.51 ± 0.09 ×10−2 | 1.33 ± 0.10 × 10−2 | – |
| 36 | – | – | <1.8×10−3 | <2.9×10−3 | <1.0×10−2 | <3.0×10−3 |
| 37 | – | – | <2.7×10−3 | 5.59 ± 0.62 × 10−3 | 6.81 ± 1.21 ×10−3 | <5.7×10−3 |
| 73 | – | – | – | – | – | – |
| 40 | – | – | 1.47± 0.31 ×10−2 | 1.05 ± 0.09 × 10−1 | – | 7.34 ± 1.29 × 10−3 |
| 43 | 1.27 ± 0.04 × 10−1 | 5.61 ± 0.81 ×10−3 | – | – | – | – |
| 18 | <8.3×10−3 | <7.4×10−3 | – | – | – | – |
| 59 | – | <4.5×10−3 | – | – | – | – |
| 60 | – | – | – | – | – | – |
| 3 | – | – | – | - | - | – |
| No. | 700183 | 700182 | 700205 | 700206 | 700207 | |
| 2019–11–25 | 2019–11–27 | 2019–12–07 | 2019–12–07 | 2019–12–08 | ||
| 71 | – | <4.4×10−3 | – | – | – | |
| 5 | – | 7.09 ± 1.45 × 10−3 | – | – | – | |
| 33 | – | – | – | – | – | |
| 35 | <3.8×10−3 | <8.9×10−3 | – | – | – | |
| 36 | <8.3×10−3 | <9.2×10−3 | – | – | – | |
| 37 | 5.61 ± 0.81 ×10−3 | – | – | – | – | |
| 73 | 3.99 ± 0.24 × 10−2 | – | – | – | – | |
| 40 | 7.21 ± 1.77 ×10−3 | – | – | – | – | |
| 43 | 1.69 ± 0.05 × 10−1 | – | – | – | – | |
| 18 | – | – | <2.7 × 10−3 | <2.6 × 10−3 | <2.2 × 10−3 | |
| 59 | – | – | <1.5 × 10−3 | <4.2 × 10−3 | <1.5 × 10−3 | |
| 60 | – | – | 1.73 ± 0.09 × 10−1 | <6.6 × 10−3 | 2.11 ± 0.11 × 10−1 | |
| 3 | – | – | <5.7 × 10−3 | <9.0 × 10−3 | <5.2×10−3 | |
Notes. Background-subtracted, PSF, and vignetting-corrected source count rates (cts s−1) are obtained from source detection and are given for the 0.2–5.0 keV band normalised to seven telescope modules. We exclude LMC X-1 here due to its brightness, which causes strong photon pile-up effects. Numbers without error and marked with “<” denote upper limits (3σ) for undetected sources in the FoV, derived from sensitivity maps produced by the eSASS task apetool.
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