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Table 2.

Best-fitting TBABS*JeTCAF model parameters for all observations of 3C 273.

OBS date. MJD MBH d h Xs R fcol χr2 Fjet Fcorona
( ×  108M) (Edd) (Edd) (rS)
2012-07-13 56121 7.6 ± 1.2 0.010 ± 0.002 0.62 ± 0.05 21.1 ± 2.9 1.69 ± 0.16 0.12 ± 0.03 1.0 2.24 ± 0.07 0.32 ± 0.01
2012-07-14 56122 7.8 ± 1.0 0.015 ± 0.001 0.71 ± 0.04 20.2 ± 2.4 2.18 ± 0.19 0.18 ± 0.01 1.0 2.33 ± 0.12 0.20 ± 0.01
2015-07-13 57216 7.3 ± 0.9 0.016 ± 0.002 0.68 ± 0.04 23.8 ± 2.6 1.89 ± 0.21 0.25 ± 0.04 1.2 1.67 ± 0.11 0.15 ± 0.01
2016-06-26 57565 7.3 ± 1.0 0.020 ± 0.003 0.86 ± 0.06 21.7 ± 2.9 3.75 ± 0.33 0.07 ± 0.02 1.3 3.80 ± 0.11 0.73 ± 0.02
2017-06-26 57930 8.1 ± 1.1 0.022 ± 0.003 0.36 ± 0.01 8.5 ± 1.0 2.17 ± 0.17 0.006 ± 0.001 1.1 1.74 ± 0.05 0.69 ± 0.02
2018-05-19 58257 8.0 ± 1.6 0.014 ± 0.001 0.77 ± 0.04 25.1 ± 2.6 2.65 ± 0.15 0.17 ± 0.02 1.1 1.68 ± 0.04 0.46 ± 0.01
2018-06-02 58271 8.1 ± 1.5 0.016 ± 0.003 0.79 ± 0.04 28.6 ± 2.4 2.64 ± 0.22 0.17 ± 0.02 1.1 1.45 ± 0.03 0.94 ± 0.02
2018-06-15 58284 8.0 ± 1.4 0.018 ± 0.002 0.78 ± 0.03 24.6 ± 2.7 2.56 ± 0.21 0.15 ± 0.01 1.0 1.30 ± 0.03 0.41 ± 0.01
2018-07-04 58303 7.8 ± 1.1 0.016 ± 0.001 0.76 ± 0.02 14.0 ± 1.3 2.86 ± 0.23 0.13 ± 0.02 1.0 1.50 ± 0.06 0.24 ± 0.01
2019-07-02 58666 8.1 ± 1.2 0.020 ± 0.002 0.79 ± 0.03 19.4 ± 2.1 3.24 ± 0.24 0.06 ± 0.01 1.1 1.24 ± 0.04 0.35 ± 0.01
2020-07-06 59036 7.2 ± 1.0 0.020 ± 0.002 0.80 ± 0.04 20.9 ± 2.0 3.36 ± 0.28 0.06 ± 0.01 1.1 1.62 ± 0.04 0.40 ± 0.01
2021-04-14 59318 8.1 ± 1.4 0.013 ± 0.001 0.71 ± 0.02 19.6 ± 2.1 1.90 ± 0.11 0.35 ± 0.05 1.1 0.17 ± 0.00 1.39 ± 0.01
2021-06-09 59374 8.1 ± 1.3 0.018 ± 0.001 0.80 ± 0.02 20.0 ± 2.3 3.17 ± 0.22 0.04 ± 0.01 1.1 1.06 ± 0.03 0.44 ± 0.01
2022-06-28 59758 8.1 ± 1.4 0.020 ± 0.003 0.81 ± 0.02 19.8 ± 2.5 3.10 ± 0.29 0.10 ± 0.02 1.1 1.24 ± 0.03 0.38 ± 0.01
2023-04-12 60046 7.9 ± 0.9 0.017 ± 0.003 0.76 ± 0.03 23.9 ± 2.6 4.69 ± 0.53 0.03 ± 0.01 1.1 1.45 ± 0.01
2024-01-07 60316 8.1 ± 1.1 0.020 ± 0.001 0.82 ± 0.01 19.8 ± 2.4 3.30 ± 0.20 0.08 ± 0.02 1.0 1.15 ± 0.03 0.49 ± 0.01

Notes. Epochs with simultaneous XMM-Newton observations showed excesses below ∼1.5 keV, which required one Gaussian component between energies 0.2–0.5 keV of width 0.1–0.4 keV and another component at ≲0.1 keV of width ∼0.4 keV. The fluxes for the jet (Fjet) and the corona (Fcorona) are in units of 10−10 erg cm−2 s−1. Here ‘–’ in Fjet denotes the lowest normalization epoch, where the total flux is taken to be the coronal flux.

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