Table 6.

The best-fitting parameters of the irradiated disc model for both epochs.

Epoch|$n_{\text{H}}\, ^{{a}}$||$E(B-V)\, ^{{b}}$||$\log _{10} \frac{L}{L_\text{Edd}}\, ^{{c}}$|f|$_{\text{out}}\, ^{{d}}$|R|$_{\text{cor}}\, ^{{e}}$||$\Gamma \, ^{{f}}$|Massg|$\log R_{\text{out}}\, ^{{h}}$|χ2/degrees of freedomi
[1022 cm−2](vega mag)[Rg][M][Rg]
10.18 ± 0.020.15 ± 0.02-0.03|$^{+0.2}_{-0.1}$|>0.87|$72^{+11}_{-7}$|1.7 ± 0.149|$^{+8}_{-12}$|5.3 ± 0.1573.3/522
20.14 ± 0.020.12 ± 0.02-0.2|$^{+0.25}_{-0.1}$|>0.8620|$^{+9}_{-3}$|2.5|$^{+0.3}_{-0.5}$|
Epoch|$n_{\text{H}}\, ^{{a}}$||$E(B-V)\, ^{{b}}$||$\log _{10} \frac{L}{L_\text{Edd}}\, ^{{c}}$|f|$_{\text{out}}\, ^{{d}}$|R|$_{\text{cor}}\, ^{{e}}$||$\Gamma \, ^{{f}}$|Massg|$\log R_{\text{out}}\, ^{{h}}$|χ2/degrees of freedomi
[1022 cm−2](vega mag)[Rg][M][Rg]
10.18 ± 0.020.15 ± 0.02-0.03|$^{+0.2}_{-0.1}$|>0.87|$72^{+11}_{-7}$|1.7 ± 0.149|$^{+8}_{-12}$|5.3 ± 0.1573.3/522
20.14 ± 0.020.12 ± 0.02-0.2|$^{+0.25}_{-0.1}$|>0.8620|$^{+9}_{-3}$|2.5|$^{+0.3}_{-0.5}$|

Note.a Hydrogen column density. b Dust reddening. c Eddington ratio. d Reprocessed fraction. e Coronal radius. f Photon index. g Calculated compact object mass (which is known to be incorrect as this ULX contains a neutron star). h Outer disc radius (NB – the compact object mass and outer disc radius were held constant for both fits; other parameters were left free to fit individual spectra). i Reduced chi-squared for the simultaneous fit of both SEDs.

Table 6.

The best-fitting parameters of the irradiated disc model for both epochs.

Epoch|$n_{\text{H}}\, ^{{a}}$||$E(B-V)\, ^{{b}}$||$\log _{10} \frac{L}{L_\text{Edd}}\, ^{{c}}$|f|$_{\text{out}}\, ^{{d}}$|R|$_{\text{cor}}\, ^{{e}}$||$\Gamma \, ^{{f}}$|Massg|$\log R_{\text{out}}\, ^{{h}}$|χ2/degrees of freedomi
[1022 cm−2](vega mag)[Rg][M][Rg]
10.18 ± 0.020.15 ± 0.02-0.03|$^{+0.2}_{-0.1}$|>0.87|$72^{+11}_{-7}$|1.7 ± 0.149|$^{+8}_{-12}$|5.3 ± 0.1573.3/522
20.14 ± 0.020.12 ± 0.02-0.2|$^{+0.25}_{-0.1}$|>0.8620|$^{+9}_{-3}$|2.5|$^{+0.3}_{-0.5}$|
Epoch|$n_{\text{H}}\, ^{{a}}$||$E(B-V)\, ^{{b}}$||$\log _{10} \frac{L}{L_\text{Edd}}\, ^{{c}}$|f|$_{\text{out}}\, ^{{d}}$|R|$_{\text{cor}}\, ^{{e}}$||$\Gamma \, ^{{f}}$|Massg|$\log R_{\text{out}}\, ^{{h}}$|χ2/degrees of freedomi
[1022 cm−2](vega mag)[Rg][M][Rg]
10.18 ± 0.020.15 ± 0.02-0.03|$^{+0.2}_{-0.1}$|>0.87|$72^{+11}_{-7}$|1.7 ± 0.149|$^{+8}_{-12}$|5.3 ± 0.1573.3/522
20.14 ± 0.020.12 ± 0.02-0.2|$^{+0.25}_{-0.1}$|>0.8620|$^{+9}_{-3}$|2.5|$^{+0.3}_{-0.5}$|

Note.a Hydrogen column density. b Dust reddening. c Eddington ratio. d Reprocessed fraction. e Coronal radius. f Photon index. g Calculated compact object mass (which is known to be incorrect as this ULX contains a neutron star). h Outer disc radius (NB – the compact object mass and outer disc radius were held constant for both fits; other parameters were left free to fit individual spectra). i Reduced chi-squared for the simultaneous fit of both SEDs.

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