Table 1.

Best-fitting model parameters obtained from the MAXI/GSC spectra.

Time [phase]Flux*Γ|${F_{\rm {scat}}}^{\dagger}$|T  in|${R_\mathrm{in}}^{\ddagger}$|χ2/d.o.f.
2.0000–3.2865[H1a]1.33 ± 0.051.58 ± 0.061.00(182)
8.0745–9.1666[H1b]6.08 ± 0.092.00 ± 0.031.02(284)
13.8187–14.5000[H1c]10.14 ± 0.152.26 ± 0.031.12(256)
18.5480–18.8500[T1]15.62|$^{+0.31}_{-0.30}$|2.50 (fixed)0.21|$^{+0.03}_{-0.02}$|1.00|$^{+0.04}_{-0.06}$|99.15|$^{+13.49}_{-8.09}$|1.106(193)
25.3756–25.9255[S1]10.87|$^{+0.43}_{-0.50}$|2.50 (fixed)0.02 ± 0.020.99 ± 0.0696.32|$^{+16.83}_{-13.59}$|0.790(96)
42.8543–44.1168[T2]8.76 ± 0.202.50 (fixed)0.18 ± 0.020.83|$^{+0.04}_{-0.05}$|116.97|$^{+18.99}_{-12.22}$|1.110(167)
48.30–49.1034[H2]5.64 ± 0.102.38 ± 0.041.236(231)
58.0–59.0[T3]5.19|$^{+0.12}_{-0.11}$|2.50 (fixed)0.07 ± 0.010.92 ± 0.0386.14|$^{+7.08}_{-7.07}$|1.05(144)
196.0–202.0 [S2]0.24|$^{+0.02}_{-0.01}$|0.00|$^{+2.50}_{-2.50}$|0.00|$^{+0.02}_{-0.00}$|0.53|$^{+0.02}_{-0.06}$|74.37|$^{+32.09}_{-7.92}$|1.115(39)
Time [phase]Flux*Γ|${F_{\rm {scat}}}^{\dagger}$|T  in|${R_\mathrm{in}}^{\ddagger}$|χ2/d.o.f.
2.0000–3.2865[H1a]1.33 ± 0.051.58 ± 0.061.00(182)
8.0745–9.1666[H1b]6.08 ± 0.092.00 ± 0.031.02(284)
13.8187–14.5000[H1c]10.14 ± 0.152.26 ± 0.031.12(256)
18.5480–18.8500[T1]15.62|$^{+0.31}_{-0.30}$|2.50 (fixed)0.21|$^{+0.03}_{-0.02}$|1.00|$^{+0.04}_{-0.06}$|99.15|$^{+13.49}_{-8.09}$|1.106(193)
25.3756–25.9255[S1]10.87|$^{+0.43}_{-0.50}$|2.50 (fixed)0.02 ± 0.020.99 ± 0.0696.32|$^{+16.83}_{-13.59}$|0.790(96)
42.8543–44.1168[T2]8.76 ± 0.202.50 (fixed)0.18 ± 0.020.83|$^{+0.04}_{-0.05}$|116.97|$^{+18.99}_{-12.22}$|1.110(167)
48.30–49.1034[H2]5.64 ± 0.102.38 ± 0.041.236(231)
58.0–59.0[T3]5.19|$^{+0.12}_{-0.11}$|2.50 (fixed)0.07 ± 0.010.92 ± 0.0386.14|$^{+7.08}_{-7.07}$|1.05(144)
196.0–202.0 [S2]0.24|$^{+0.02}_{-0.01}$|0.00|$^{+2.50}_{-2.50}$|0.00|$^{+0.02}_{-0.00}$|0.53|$^{+0.02}_{-0.06}$|74.37|$^{+32.09}_{-7.92}$|1.115(39)

*2–20 keV X-ray flux in the units of × 10−8 erg cm−2 s−1.

Scattering fraction.

Inner radius estimated from the normalization of diskbb by assuming a distance and inclination of 10 kpc and 0°, respectively.

Table 1.

Best-fitting model parameters obtained from the MAXI/GSC spectra.

Time [phase]Flux*Γ|${F_{\rm {scat}}}^{\dagger}$|T  in|${R_\mathrm{in}}^{\ddagger}$|χ2/d.o.f.
2.0000–3.2865[H1a]1.33 ± 0.051.58 ± 0.061.00(182)
8.0745–9.1666[H1b]6.08 ± 0.092.00 ± 0.031.02(284)
13.8187–14.5000[H1c]10.14 ± 0.152.26 ± 0.031.12(256)
18.5480–18.8500[T1]15.62|$^{+0.31}_{-0.30}$|2.50 (fixed)0.21|$^{+0.03}_{-0.02}$|1.00|$^{+0.04}_{-0.06}$|99.15|$^{+13.49}_{-8.09}$|1.106(193)
25.3756–25.9255[S1]10.87|$^{+0.43}_{-0.50}$|2.50 (fixed)0.02 ± 0.020.99 ± 0.0696.32|$^{+16.83}_{-13.59}$|0.790(96)
42.8543–44.1168[T2]8.76 ± 0.202.50 (fixed)0.18 ± 0.020.83|$^{+0.04}_{-0.05}$|116.97|$^{+18.99}_{-12.22}$|1.110(167)
48.30–49.1034[H2]5.64 ± 0.102.38 ± 0.041.236(231)
58.0–59.0[T3]5.19|$^{+0.12}_{-0.11}$|2.50 (fixed)0.07 ± 0.010.92 ± 0.0386.14|$^{+7.08}_{-7.07}$|1.05(144)
196.0–202.0 [S2]0.24|$^{+0.02}_{-0.01}$|0.00|$^{+2.50}_{-2.50}$|0.00|$^{+0.02}_{-0.00}$|0.53|$^{+0.02}_{-0.06}$|74.37|$^{+32.09}_{-7.92}$|1.115(39)
Time [phase]Flux*Γ|${F_{\rm {scat}}}^{\dagger}$|T  in|${R_\mathrm{in}}^{\ddagger}$|χ2/d.o.f.
2.0000–3.2865[H1a]1.33 ± 0.051.58 ± 0.061.00(182)
8.0745–9.1666[H1b]6.08 ± 0.092.00 ± 0.031.02(284)
13.8187–14.5000[H1c]10.14 ± 0.152.26 ± 0.031.12(256)
18.5480–18.8500[T1]15.62|$^{+0.31}_{-0.30}$|2.50 (fixed)0.21|$^{+0.03}_{-0.02}$|1.00|$^{+0.04}_{-0.06}$|99.15|$^{+13.49}_{-8.09}$|1.106(193)
25.3756–25.9255[S1]10.87|$^{+0.43}_{-0.50}$|2.50 (fixed)0.02 ± 0.020.99 ± 0.0696.32|$^{+16.83}_{-13.59}$|0.790(96)
42.8543–44.1168[T2]8.76 ± 0.202.50 (fixed)0.18 ± 0.020.83|$^{+0.04}_{-0.05}$|116.97|$^{+18.99}_{-12.22}$|1.110(167)
48.30–49.1034[H2]5.64 ± 0.102.38 ± 0.041.236(231)
58.0–59.0[T3]5.19|$^{+0.12}_{-0.11}$|2.50 (fixed)0.07 ± 0.010.92 ± 0.0386.14|$^{+7.08}_{-7.07}$|1.05(144)
196.0–202.0 [S2]0.24|$^{+0.02}_{-0.01}$|0.00|$^{+2.50}_{-2.50}$|0.00|$^{+0.02}_{-0.00}$|0.53|$^{+0.02}_{-0.06}$|74.37|$^{+32.09}_{-7.92}$|1.115(39)

*2–20 keV X-ray flux in the units of × 10−8 erg cm−2 s−1.

Scattering fraction.

Inner radius estimated from the normalization of diskbb by assuming a distance and inclination of 10 kpc and 0°, respectively.

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