Table 1: Best-fitting parameters for the spectral fits to the extended jet-associated emission.
Model^(a) $N^{{(b)}}_{\rm H}$ kT $\Gamma^{{(c)}}$ $F_{\rm abs}^{{(d)}}$ $F_{\rm unabs}^{{(d)}}$ $\chi^2_{\rm red}$ ( $\chi^2$ /d.o.f.)

[10²² cm^-2] [keV] [erg s^-1 cm^-2] [erg s^-1 cm^-2]

(R&S) $^{\rm abs}$ $\rm0.49_{-0.06}^{+0.08}$ $\rm0.48_{-0.08}^{+0.08}$ - $0.8\times 10^{-13}$ $3.9\times 10^{-13}$ 0.49 (10.8/22)

(M&K) $^{\rm abs}$ $\rm0.41_{-0.06}^{+0.08}$ $\rm0.41_{-0.07}^{+0.09}$ - $0.7\times 10^{-13}$ $3.4\times 10^{-13}$ 0.53 (11.6/22)

(PL) $^{\rm abs}$ $\rm0.06_{-0.02}^{+0.07}$ - $\rm 3.8_{-0.7}^{+0.6}$ $1.5\times 10^{-13}$ $2.0\times 10^{-13}$ 0.52 (11.5/22)

^a R&S: Raymond/Smith plasma, M&K: Mewe/Kaastra plasma, PL: power-law; ^b absorbing column density; $2\times 10^{20}$ cm^-2 is set as a lower limit; ^c photon index; ^d (un)absorbed X-ray flux between 0.2 keV and 8.0 keV.

**Table 1:** Best-fitting parameters for the spectral fits to the extended jet-associated emission.
Model^(a)	$N^{{(b)}}_{\rm H}$	kT	$\Gamma^{{(c)}}$	$F_{\rm abs}^{{(d)}}$	$F_{\rm unabs}^{{(d)}}$	$\chi^2_{\rm red}$ ( $\chi^2$ /d.o.f.)
	[10²² cm^-2]	[keV]		[erg s^-1 cm^-2]	[erg s^-1 cm^-2]
(R&S) $^{\rm abs}$	$\rm0.49_{-0.06}^{+0.08}$	$\rm0.48_{-0.08}^{+0.08}$	-	$0.8\times 10^{-13}$	$3.9\times 10^{-13}$	0.49 (10.8/22)
(M&K) $^{\rm abs}$	$\rm0.41_{-0.06}^{+0.08}$	$\rm0.41_{-0.07}^{+0.09}$	-	$0.7\times 10^{-13}$	$3.4\times 10^{-13}$	0.53 (11.6/22)
(PL) $^{\rm abs}$	$\rm0.06_{-0.02}^{+0.07}$	-	$\rm 3.8_{-0.7}^{+0.6}$	$1.5\times 10^{-13}$	$2.0\times 10^{-13}$	0.52 (11.5/22)

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