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Table 2.

Best-fitted parameters of the pre-burst persistent spectra.

NICER NH Tin Kdiskbb kTbb Kbb χν2 (d.o.f.) Fper(a)
(Obs. Id) (1022 cm−2) (keV) (keV) (10−9 erg s−1 cm−2)
6203670101 0.75 ± 0.05 159 36 + 45 $ 159_{-36}^{+45} $ 1.79 ± 0.06 26 ± 3 1.02(107) 3.96 ± 0.03
6203670101 0.79 ± 0.07 135 35 + 44 $ 135_{-35}^{+44} $ 1.74 ± 0.07 28 ± 4 1.01(107) 3.99 ± 0.03
6203670101 0.85 ± 0.07 120 29 + 36 $ 120_{-29}^{+36} $ 1.82 ± 0.07 25 ± 4 1.16(109) 4.47 ± 0.03
6203670106 2.29 ± 0.03 0.99 ± 0.07 188 37 + 43 $ 188_{-37}^{+43} $ 1.72 ± 0.08 44 ± 9 1.11(118) 8.20 ± 0.03
6203670115 0.74 ± 0.03 333 52 + 61 $ 333_{-52}^{+61} $ 1.50 ± 0.05 35 ± 6 0.86(115) 4.26 ± 0.03
6203670119 0.60 ± 0.02 326 55 + 67 $ 326_{-55}^{+67} $ 1.43 ± 0.06 15 ± 2 0.96(104) 1.65 ± 0.03
6203670120 0.65 ± 0.03 197 37 + 46 $ 197_{-37}^{+46} $ 2.32 ± 0.26 3 ± 0.8 0.84(101) 1.73 ± 0.03

Notes.

(a)

The unabsorbed bolometric persistent flux in 0.1 − 250 keV.

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