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Table 3:

ACIS-S best-fit parameters and results for the spatially-resolved regions of NGC 5252.

Region
$N_{\rm H}$a $\Gamma$b kTc $E_{\rm c}$d EWe $F_{\rm0.5-2 ~keV}$f $F_{\rm 2-10~ keV}$f $L_{\rm0.5-2 ~keV}$g $L_{\rm 2-10~ keV}$g $\chi^2/\nu$
  (1022 cm-2)   (eV) (keV) (eV)          
Nucleus $2.32 \pm^{0.13}_{0.15}$ $1.00 \pm^{0.08}_{0.06}$ $140\pm^{60}_{40}$ $6.37 \pm^{0.06}_{0.05}$ $50 \pm 20$ $2.66\pm^{0.11}_{0.28}$ $103\pm^2_3$ $0.82\pm^{0.03}_{0.09}$ $1130 \pm^{20}_{30}$ 176.9/127
SENS $0.47\pm^{0.16}_{0.31}$ $0.8 \pm 0.4$ <140 ... ... $0.06 \pm 0.05$ $0.34 \pm^{0.08}_{0.14}$ $50 \pm 40$ $4.1 \pm^{1.0}_{1.7}$ 3.0/5
NS $\equiv$ $N_{\rm H,Gal}$ $-0.9\pm^{0.5}_{0.6}$ $240 \pm^{40}_{30}$ ... ... $0.066\pm^{0.011}_{0.015}$ $1.3 \pm 0.3$ $0.89 \pm^{0.15}_{0.20}$ $15 \pm 3$ 1.0/3
SS $\equiv$ $N_{\rm H,Gal}$ $0.0 \pm 0.4$ $110\pm^{13}_{21}$ ... ... $0.122 \pm^{0.017}_{0.023}$ $0.70 \pm^{0.18}_{0.53}$ $1.7 \pm^{0.2}_{0.3}$ $8 \pm^2_6$ 5.1/7
      $510\pm^{170}_{230}$              

Notes.  (a) Absorbing column density; (b) photon index; (c) temperature of the emitting thermal gas derived using mekal to fit the spatially resolved data; (d) energy of the emission line; (e) equivalent width; (f) flux in units of 10-13 erg s-1 cm-2; (g) luminosity in units of 1040 erg s-1.


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