Table C.1.
Fit results to the XMM-Newton quiescent spectra of RX J1301.9+2747
model | kTdisk | log Ndisk | kT | log N | Γ | log Npow | NH | log𝒵 | AIC | f0.3 − 2 | f2 − 10 | L0.3 − 2 keV | L2 − 10 keV | LBOL |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) |
Epoch: 2000 | ||||||||||||||
0 |
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- | - | - | - | < 0.2 | −3.4 | −1.7 |
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- |
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- |
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1 |
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- | - | < 0.5 | −2.5 | 0 |
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< 0.01 |
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< 0.02 |
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2 |
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- | - |
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< 0.2 | −3.9 | −4.2 |
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< 0.11 |
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< 0.14 |
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3 |
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< 0.6 | 0 | −4.0 |
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< 0.04 |
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< 0.06 |
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4 |
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− | − | < 0.3 | −0.4 | −1.0 |
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< 0.06 |
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< 0.08 |
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Epoch: 2019 | ||||||||||||||
0 |
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- | - | - | - | < 0.4 | −50.9 | −52.3 |
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- |
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- |
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1 |
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- | - | < 3.2 | −2.62 | 0 |
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2 |
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- | - |
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< 2.1 | −8.5 | −6.7 |
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3 |
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< 1.6 | 0 | −3.9 |
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4 |
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− | − | < 1.4 | −7.2 | −3.2 |
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Epoch: 2020 | ||||||||||||||
0 |
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- | - | - | - | < 0.1 | −223.6 | −224.6 |
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- |
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- |
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1 |
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- | - | < 0.2 | −3.0 | 0 |
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2 |
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- | - |
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< 0.4 | −4.2 | −2.1 |
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3 |
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200+10−10 |
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< 0.2 | 0 | −3.9 |
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4 |
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− | − | < 0.5 | −4.3 | 0 |
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Epoch: 2022A | ||||||||||||||
0 |
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- | - | - | - | < 0.1 | −90.3 | −91.9 |
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- |
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- |
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1 |
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- | - | < 0.2 | −2.7 | −1.0 |
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2 |
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- | - |
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< 0.5 | −1.8 | −1.4 |
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3 |
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< 0.2 | 0 | −4.75 |
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4 |
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− | − | < 0.3 | −1.8 | 0 |
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Epoch: 2022B | ||||||||||||||
0 |
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- | - | - | - | < 0.1 | −177.2 | −179.4 |
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- |
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- |
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1 |
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- | - | < 0.2 | −2.7 | −1.1 |
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2 |
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- | - |
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< 1.2 | −1.7 | −1.0 |
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3 |
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< 0.2 | 0 | −5.3 |
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4 |
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− | − | < 0.3 | −1.8 | 0 |
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Notes. Col. (1) model adopted, model 0: [diskbb]; model 1: [diskbb + bbody]; model 2: [diskbb + powerlaw]; model 3: [diskbb + bbody + powerlaw]; model 4: [diskbb + compTT]. Col. (2) diskbb inner temperature (eV). Col. (3) logarithm of the diskbb normalization. Col. (4) bbody or compTT temperature (eV). Col. (5) logarithm of the bbody or compTT normalization. Col. (6) powerlaw photon index. Col. (7) logarithm of the powerlaw normalization. Col. (8) absorbing column density (1020 cm−2). Col. (9) logarithm of the Bayesian evidence normalized to the maximum value. Col. (10) Akaike Information Criterium AIC = C − 2 × m, where C is the likelihood and m is the number of degrees of freedom, normalized to the maximum value. Col. (11) observed flux in the 0.3 − 2 keV band (10−13 erg cm−2 s−1). Col. (12) observed flux in the 2 − 10 keV band (10−15 erg cm−2 s−1). Col. (13) intrinsic luminosity computed in the 0.3 − 2 keV band (1042 erg s−1). Col. (14) intrinsic luminosity computed in the 2 − 10 keV band (1039 erg s−1). Col (15) total bolometric luminosity of the model (1042 erg s−1).
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