X-ray spectral fit results inferred using bxa, with the abbreviated model names representing the tbabs*zbbody, tbabs*zpwrlaw, tbabs*zabsbb, tbabs*zabspwrlaw, and tbabs*zbremss models, respectively (defined in Section 3.5). The kT columns are in units of keV and NH in 1022 cm−2. |$\Delta \mathcal {Z}$| is provided for each fitted source model, and it is defined as the log of the evidence ratio between that model and the model with the highest evidence in the row, |$\Delta \mathcal {Z} = 0$| therefore indicates that a model is the ‘best fitting’ to the observed X-ray spectrum. The lower the value of |$\Delta \mathcal {Z}$|, the more strongly this model is disfavoured relative to the best-fitting model.
| MJD . | OBSID . | zbb . | zpo . | zabsbb . | zabspo . | zbrems . | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |$\Delta \mathcal {Z}$| | kT | |$\Delta \mathcal {Z}$| | Γ | |$\Delta \mathcal {Z}$| | NH | kT | |$\Delta \mathcal {Z}$| | NH | Γ | |$\Delta \mathcal {Z}$| | kTp | ||
| 59143.580 | eRASS2 | −4.3 | |$0.10 ^{0.01}_{0.01}$| | 0.0 | |$4.0 ^{0.2}_{0.3}$| | −8.6 | |$0.01 ^{0.01}_{0.00}$| | |$0.10 ^{0.01}_{0.01}$| | −1.7 | |$0.02 ^{0.02}_{0.01}$| | |$4.4 ^{0.4}_{0.3}$| | −1.3 | |$0.22 ^{0.03}_{0.02}$| |
| 59212.289 | 00013855008 | −7.6 | |$0.15 ^{0.02}_{0.02}$| | 0.0 | |$3.8 ^{0.4}_{0.4}$| | −9.8 | |$0.02 ^{0.03}_{0.01}$| | |$0.14 ^{0.02}_{0.02}$| | −1.4 | |$0.04 ^{0.08}_{0.03}$| | |$4.2 ^{0.7}_{0.5}$| | −2.3 | |$0.41 ^{0.11}_{0.08}$| |
| 59220.631 | 00013855009 | 0.0 | |$0.14 ^{0.02}_{0.01}$| | −3.9 | |$3.7 ^{0.4}_{0.4}$| | −0.8 | |$0.08 ^{0.17}_{0.06}$| | |$0.13 ^{0.02}_{0.02}$| | −1.2 | |$0.42 ^{0.16}_{0.19}$| | |$6.7 ^{1.0}_{1.4}$| | −1.0 | |$0.35 ^{0.08}_{0.06}$| |
| MJD . | OBSID . | zbb . | zpo . | zabsbb . | zabspo . | zbrems . | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |$\Delta \mathcal {Z}$| | kT | |$\Delta \mathcal {Z}$| | Γ | |$\Delta \mathcal {Z}$| | NH | kT | |$\Delta \mathcal {Z}$| | NH | Γ | |$\Delta \mathcal {Z}$| | kTp | ||
| 59143.580 | eRASS2 | −4.3 | |$0.10 ^{0.01}_{0.01}$| | 0.0 | |$4.0 ^{0.2}_{0.3}$| | −8.6 | |$0.01 ^{0.01}_{0.00}$| | |$0.10 ^{0.01}_{0.01}$| | −1.7 | |$0.02 ^{0.02}_{0.01}$| | |$4.4 ^{0.4}_{0.3}$| | −1.3 | |$0.22 ^{0.03}_{0.02}$| |
| 59212.289 | 00013855008 | −7.6 | |$0.15 ^{0.02}_{0.02}$| | 0.0 | |$3.8 ^{0.4}_{0.4}$| | −9.8 | |$0.02 ^{0.03}_{0.01}$| | |$0.14 ^{0.02}_{0.02}$| | −1.4 | |$0.04 ^{0.08}_{0.03}$| | |$4.2 ^{0.7}_{0.5}$| | −2.3 | |$0.41 ^{0.11}_{0.08}$| |
| 59220.631 | 00013855009 | 0.0 | |$0.14 ^{0.02}_{0.01}$| | −3.9 | |$3.7 ^{0.4}_{0.4}$| | −0.8 | |$0.08 ^{0.17}_{0.06}$| | |$0.13 ^{0.02}_{0.02}$| | −1.2 | |$0.42 ^{0.16}_{0.19}$| | |$6.7 ^{1.0}_{1.4}$| | −1.0 | |$0.35 ^{0.08}_{0.06}$| |
X-ray spectral fit results inferred using bxa, with the abbreviated model names representing the tbabs*zbbody, tbabs*zpwrlaw, tbabs*zabsbb, tbabs*zabspwrlaw, and tbabs*zbremss models, respectively (defined in Section 3.5). The kT columns are in units of keV and NH in 1022 cm−2. |$\Delta \mathcal {Z}$| is provided for each fitted source model, and it is defined as the log of the evidence ratio between that model and the model with the highest evidence in the row, |$\Delta \mathcal {Z} = 0$| therefore indicates that a model is the ‘best fitting’ to the observed X-ray spectrum. The lower the value of |$\Delta \mathcal {Z}$|, the more strongly this model is disfavoured relative to the best-fitting model.
| MJD . | OBSID . | zbb . | zpo . | zabsbb . | zabspo . | zbrems . | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |$\Delta \mathcal {Z}$| | kT | |$\Delta \mathcal {Z}$| | Γ | |$\Delta \mathcal {Z}$| | NH | kT | |$\Delta \mathcal {Z}$| | NH | Γ | |$\Delta \mathcal {Z}$| | kTp | ||
| 59143.580 | eRASS2 | −4.3 | |$0.10 ^{0.01}_{0.01}$| | 0.0 | |$4.0 ^{0.2}_{0.3}$| | −8.6 | |$0.01 ^{0.01}_{0.00}$| | |$0.10 ^{0.01}_{0.01}$| | −1.7 | |$0.02 ^{0.02}_{0.01}$| | |$4.4 ^{0.4}_{0.3}$| | −1.3 | |$0.22 ^{0.03}_{0.02}$| |
| 59212.289 | 00013855008 | −7.6 | |$0.15 ^{0.02}_{0.02}$| | 0.0 | |$3.8 ^{0.4}_{0.4}$| | −9.8 | |$0.02 ^{0.03}_{0.01}$| | |$0.14 ^{0.02}_{0.02}$| | −1.4 | |$0.04 ^{0.08}_{0.03}$| | |$4.2 ^{0.7}_{0.5}$| | −2.3 | |$0.41 ^{0.11}_{0.08}$| |
| 59220.631 | 00013855009 | 0.0 | |$0.14 ^{0.02}_{0.01}$| | −3.9 | |$3.7 ^{0.4}_{0.4}$| | −0.8 | |$0.08 ^{0.17}_{0.06}$| | |$0.13 ^{0.02}_{0.02}$| | −1.2 | |$0.42 ^{0.16}_{0.19}$| | |$6.7 ^{1.0}_{1.4}$| | −1.0 | |$0.35 ^{0.08}_{0.06}$| |
| MJD . | OBSID . | zbb . | zpo . | zabsbb . | zabspo . | zbrems . | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |$\Delta \mathcal {Z}$| | kT | |$\Delta \mathcal {Z}$| | Γ | |$\Delta \mathcal {Z}$| | NH | kT | |$\Delta \mathcal {Z}$| | NH | Γ | |$\Delta \mathcal {Z}$| | kTp | ||
| 59143.580 | eRASS2 | −4.3 | |$0.10 ^{0.01}_{0.01}$| | 0.0 | |$4.0 ^{0.2}_{0.3}$| | −8.6 | |$0.01 ^{0.01}_{0.00}$| | |$0.10 ^{0.01}_{0.01}$| | −1.7 | |$0.02 ^{0.02}_{0.01}$| | |$4.4 ^{0.4}_{0.3}$| | −1.3 | |$0.22 ^{0.03}_{0.02}$| |
| 59212.289 | 00013855008 | −7.6 | |$0.15 ^{0.02}_{0.02}$| | 0.0 | |$3.8 ^{0.4}_{0.4}$| | −9.8 | |$0.02 ^{0.03}_{0.01}$| | |$0.14 ^{0.02}_{0.02}$| | −1.4 | |$0.04 ^{0.08}_{0.03}$| | |$4.2 ^{0.7}_{0.5}$| | −2.3 | |$0.41 ^{0.11}_{0.08}$| |
| 59220.631 | 00013855009 | 0.0 | |$0.14 ^{0.02}_{0.01}$| | −3.9 | |$3.7 ^{0.4}_{0.4}$| | −0.8 | |$0.08 ^{0.17}_{0.06}$| | |$0.13 ^{0.02}_{0.02}$| | −1.2 | |$0.42 ^{0.16}_{0.19}$| | |$6.7 ^{1.0}_{1.4}$| | −1.0 | |$0.35 ^{0.08}_{0.06}$| |
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