Table 5
Parameters used for the SSC modelling of the SED of 1RXS J101015.9 − 311909 and derived physical quantities.
| Fermi>300 MeV | Fermi>1 GeV | |||
| Case A | Case B | Case A | Case B | |
|
|
||||
| γe,break | 1.08 × 105 | 9.0 × 104 | 1.01 × 105 | 7.8 × 104 |
| α1 | 2.2 | 2.2 | 2.0 | 2.0 |
| K | 5.67 × 104 | 3.37 × 102 | 6.6 × 103 | 4.5 × 101 |
| ue | 5.37 × 10-2 | 3.15 × 10-4 | 3.42 × 10-2 | 2.24 × 10-4 |
|
|
||||
| B | 0.16 | 0.025 | 0.16 | 0.025 |
| uB | 1.02 × 10-3 | 2.49 × 10-5 | 1.02 × 10-3 | 2.49 × 10-5 |
| ue/uB | 52.7 | 12.7 | 33.6 | 9.0 |
| R | 2.37 × 1015 | 7 × 1016 | 2.37 × 1015 | 7 × 1016 |
| τvar | 0.8 | 24.7 | 0.8 | 24.7 |
| Ljet | 7.6 × 1042 | 4.1 × 1043 | 4.9 × 1042 | 3.0 × 1043 |
Notes. Summary of the SED parameters for the two Fermi/LAT spectra considered (low-energy threshold equal to 300 MeV and 1 GeV) and for the two cases proposed in the Swift/XRT analysis (case A and case B). For all the cases considered, the minimum and maximum Lorentz factors of the electron distribution are set to γe,min = 300 and γe,max = 5 × 106 respectively; the angle to the line of sight is θ = 1°, the Doppler factor is δ = 30, and the index of the electron distribution after the break is α2 = 4.0. The electron-distribution normalization parameter K is in units of cm-3; the magnetic field B is in G; the emitting-region size R is in cm; the energy densities ue,B are in erg cm-3; the variability timescale τvar is in hours and the jet luminosity Ljet is in ergs s-1.
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