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Table 2.

Observation details and results of the XSPEC and BEHR analysis.

Source Obs. ID Net exposure [ks] Flux log(LX, Observed) log(LX, Predicted)

pn MOS1 MOS2 [10−16 erg s cm−2] [erg s−1] [erg s−1]
BB1 0865260101 14.7 21.8 21.8 63 ± 9 40.5 ± 0.3 41.0
BB2 0865260201 38.0 53.8 53.8 < 8.1 < 39.3 40.4
BB3 0865260301 16.6 23.3 23.3 < 9.5 < 40.2 41.0
BB4 0865260401 24.7 30.8 30.7 < 2.1 < 39.7 41.0
BB5 0865260501 5.1 9.9 8.9 < 1.5 < 39.9 40.4
BB7 0865260701 23.5 43.9 43.9 < 4.5 < 39.5 40.2
BB8 0865260801 50.7 59.7 59.7 68 ± 8 40.4 ± 0.2 39.9

Notes. Rest frame fluxes and luminosities (or their upper limits) in the 0.5–8 keV band along with the predicted luminosity values calculated using the Brorby et al. (2016) scaling relation. For the two detected sources, the fluxes were determined with the use of the XSPEC software. For the rest, the upper limits on fluxes were measured using the BEHR code and the WebPIMMS flux estimate.

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