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Table 1.

Computed BW model parameters.

OBSID MJD Lx (× 1037 erg s−1) α σ/σT σ ¯ / σ T $ {\overline\sigma}/{\sigma_{\text{T}}} $ (× 10−4) J (× 107) Tth (× 107 K) vth/c τth τmax τtrap
P0514361017 59955.509 0.28 ± 0.04 0.457 3.572 × 10−2 381.22 0.69 0.81 0.009 0.019 0.265 1.48
P0514361022 59961.859 1.14 ± 0.08 0.536 0.018 × 10−2 2.23 23.14 2.86 0.019 0.036 0.016 1.37
P0514361025 59965.369 1.26 ± 0.02 5.528 3.353 × 10−8 0.11 2085 12.3 0.037 0.007 2 × 10−5 0.43
P0514361035 59973.111 2.27 ± 0.02 5.417 0.895 × 10−8 0.046 4119 16.23 0.046 0.009 1 × 10−5 0.43
P0514361038 59977.804 2.22 ± 0.01 5.597 0.989 × 10−8 0.073 3791 15.50 0.045 0.008 1 × 10−5 0.42
P0514361045 59987.917 2.40 ± 0.22 1.833 0.012 × 10−5 0.068 3304 14.86 0.043 0.024 0.12 × 10−3 0.74
P0514361049 59992.480 2.50 ± 0.14 2.080 0.146 × 10−5 1.03 166 5.58 0.027 0.013 0.37 × 10−3 0.69
P0514361057 60005.769 1.62 ± 0.08 3.850 0.031 × 10−2 468.15 0.46 0.75 0.009 0.002 2.94 × 10−3 0.51
P0514361067 60021.773 0.50 ± 0.01 3.072 0.267 × 10−2 2702.5 0.19 0.53 0.007 0.002 0.011 0.57
P0514361074 60029.248 0.36 ± 0.02 0.590 3.398 × 10−2 471.85 0.34 0.65 0.008 0.014 0.200 1.30

Notes. The source luminosity, Lx, is estimated in 1–120 keV, in units of 1037 erg s−1. The distance to the source is assumed to be 2.44 kpc (Bailer-Jones et al. 2021). The accretion mass flux, J, is in units of g s−1 cm−2.

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