Table 6: Spectral fitting results for NGC3690.
Parameter Power-law Single Temperature Double Temperature Raymond Smith + Triple temperature cevmekl cevmekl +
Raymond-Smith Raymond Smith Power-law Raymond Smith power-law
kT (KeV) 4.25-0.45+0.36subscriptsuperscript4.250.360.454.25^{+0.36}_{-0.45} 0.83-0.03+0.03subscriptsuperscript0.830.030.030.83^{+0.03}_{-0.03} 0.83-0.04+0.02subscriptsuperscript0.830.020.040.83^{+0.02}_{-0.04} 0.285-0.063+0.187subscriptsuperscript0.2850.1870.0630.285^{+0.187}_{-0.063} 57.08(>30)annotated57.08absent3057.08(>30)
10.3-2.4+5.9subscriptsuperscript10.35.92.410.3^{+5.9}_{-2.4} 0.871-0.676+0.427subscriptsuperscript0.8710.4270.6760.871^{+0.427}_{-0.676}
11.17-3.13+6.96subscriptsuperscript11.176.963.1311.17^{+6.96}_{-3.13}
ΓΓ\Gamma 2.23-0.12+0.12subscriptsuperscript2.230.120.122.23^{+0.12}_{-0.12} 1.56-0.11+0.11subscriptsuperscript1.560.110.111.56^{+0.11}_{-0.11} 1.52-0.12+0.13subscriptsuperscript1.520.130.121.52^{+0.13}_{-0.12}
αsuperscript𝛼\alpha^{{\dagger}} 0.22-0.01+0.11subscriptsuperscript0.220.110.010.22^{+0.11}_{-0.01} 1.01.01.0
NH(1020cm-2)subscript𝑁𝐻superscript1020𝑐superscript𝑚2N_{H}(10^{20}cm^{-2}) 5.50-0.7+0.7subscriptsuperscript5.500.70.75.50^{+0.7}_{-0.7} 2.11-0.33+0.38subscriptsuperscript2.110.380.332.11^{+0.38}_{-0.33} 1.60-0.40+0.42subscriptsuperscript1.600.420.401.60^{+0.42}_{-0.40} 2.42-0.46+0.63subscriptsuperscript2.420.630.462.42^{+0.63}_{-0.46} 2.031-0.472+0.283subscriptsuperscript2.0310.2830.4722.031^{+0.283}_{-0.472} 3.21-0.48+0.73subscriptsuperscript3.210.730.483.21^{+0.73}_{-0.48} 2.910.55+0.68subscriptsuperscript2.910.680.552.91^{+0.68}_{0.55}
χ2superscript𝜒2\chi^{2} / d.o.f. 490.0/242 624.5/242624.5242624.5/242 287.8/235287.8235287.8/235 291.5/235291.5235291.5/235 290.3/237290.3237290.3/237 309.9/241309.9241309.9/241 286.4/235286.4235286.4/235
Flux{}^{{\ddagger}} (0.1-2.0keV) 9.72 8.85 8.5 9.0 8.95 8.62 8.2
Flux{}^{{\ddagger}} (2.0-10.0keV) 7.68 9.59 10.8 10.8 10.3 9.9 10.8
Total Luminosity{}^{\ast} (0.1-10.0keV) 8.3 8.8 9.2 9.46 9.2

{\dagger} The slope of power-law distribution of temperatures in the cevmekl model.
{\ddagger} The fluxes are in units of 10-13ergs-1cm-2superscript1013ergsuperscripts1superscriptcm210^{-13}\rm{erg\,s^{-1}\,cm^{-2}} .
\ast The luminosity is in units of 1041ergs-1superscript1041ergsuperscripts110^{41}\rm{erg\,s^{-1}} .