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Table 4.

Parameters of the non-interacting two-zone model.

State Epoch Model R δ B n1 n2 γmin γb γmax N* Le σ z χ2
[MJD] (region) [×1015 cm] [G] [×103] [×104] [×106] [×103 cm−3] [erg/s] (points)
A 58903.5-58905.5 2-zone (blob) 13 11 0.10 1.70 3.4 1.00 25 2.0 1.2 1.8 × 1044 4.3 × 10−3 0.18 152.2
2-zone (core) 370 11 0.13 1.64 2.7 0.35 0.11 0.2 2.5 6.2 × 1043 16 0.18 (33)

B 58905.5-58907.5 2-zone (blob) 13 11 0.20 1.70 3.4 1.00 10 1.0 0.8 8.2× 1043 3.7× 102 0.18 334.9
2-zone (core) 370 11 0.13 1.64 2.7 0.35 0.11 0.2 2.5 6.2 × 1043 16 0.18 (30)

C 58907.5-58908.5 2-zone (blob) 13 11 0.11 1.70 3.4 1.00 30 1.5 0.11 1.7× 1044 5.4× 103 0.18 24.6
2-zone (core) 370 11 0.13 1.64 2.7 0.35 0.11 0.2 2.5 6.2 × 1043 16 0.18 (23)

D 58908.5-58909.5 2-zone (blob) 13 11 0.08 1.70 3.4 1.00 30 2.0 2.0 3.1× 1044 1.6× 103 0.18 266.1
2-zone (core) 370 11 0.13 1.64 2.7 0.35 0.11 0.2 2.5 6.2 × 1043 16 0.18 (28)

Notes. Columns: (1) State. (2) Epoch. (3) Model (emission region). (4) Radius of the emission region. (5) Doppler factor. (6) Magnetic field strength. (7) and (8) Slopes of the electron spectrum around γb. (9) Minimum electron Lorentz factor. (10) Break electron Lorentz factor. (11) Maximum electron Lorentz factor. (12) Electron density. (13) Electron luminosity. (14) Jet magnetisation given as the ratio of the Poynting luminosity (Celotti & Ghisellini 2008) to the total particle luminosity, LB/Le. (15) Redshift. (16) Sum of squared residuals normalised by the uncertainties on the flux points (χ2), excluding the radio band. The number of flux points is reported in parenthesis. In bold are parameters that changed compared to state A.

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