Table D2.

The 5 best matching spectral models for accelerator SNR G8.7−0.1 for an age of 28 kyr with their model parameters.

ModelαχδδpEp, maxSN TypeMejESNWpEp, escχ2/mS
name(PeV)(M)(erg)(1050 erg)(TeV)(Spectral)(Spatial, 10−13)
G1b1.80.010.61.45.0Ia110511.56.20.61.9
G2b*1.80.10.41.45.0Ia110511.56.20.81.6
G3b1.80.0010.41.41.0II2010521.08.11.02.3
G4b2.00.0010.41.45.0II1010520.718.11.03.2
G5b1.80.10.41.41.0II2010521.08.11.02.0
ModelαχδδpEp, maxSN TypeMejESNWpEp, escχ2/mS
name(PeV)(M)(erg)(1050 erg)(TeV)(Spectral)(Spatial, 10−13)
G1b1.80.010.61.45.0Ia110511.56.20.61.9
G2b*1.80.10.41.45.0Ia110511.56.20.81.6
G3b1.80.0010.41.41.0II2010521.08.11.02.3
G4b2.00.0010.41.45.0II1010520.718.11.03.2
G5b1.80.10.41.41.0II2010521.08.11.02.0

Note.* Best spatial model

Table D2.

The 5 best matching spectral models for accelerator SNR G8.7−0.1 for an age of 28 kyr with their model parameters.

ModelαχδδpEp, maxSN TypeMejESNWpEp, escχ2/mS
name(PeV)(M)(erg)(1050 erg)(TeV)(Spectral)(Spatial, 10−13)
G1b1.80.010.61.45.0Ia110511.56.20.61.9
G2b*1.80.10.41.45.0Ia110511.56.20.81.6
G3b1.80.0010.41.41.0II2010521.08.11.02.3
G4b2.00.0010.41.45.0II1010520.718.11.03.2
G5b1.80.10.41.41.0II2010521.08.11.02.0
ModelαχδδpEp, maxSN TypeMejESNWpEp, escχ2/mS
name(PeV)(M)(erg)(1050 erg)(TeV)(Spectral)(Spatial, 10−13)
G1b1.80.010.61.45.0Ia110511.56.20.61.9
G2b*1.80.10.41.45.0Ia110511.56.20.81.6
G3b1.80.0010.41.41.0II2010521.08.11.02.3
G4b2.00.0010.41.45.0II1010520.718.11.03.2
G5b1.80.10.41.41.0II2010521.08.11.02.0

Note.* Best spatial model

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