Table A.4
Best-fit parameters of spectral analysis for 2001, 2002 and 2009 with XMM-Newton observations of NGC 4051 in 0.2–10 keV energy rangea.
| Observational | kTs | α = | log (A) |  |
Eline |  |
Ec | kTpl |  |
 |
|---|---|---|---|---|---|---|---|---|---|---|
| ID | (keV) | Γ − 1 | (keV) | (keV) | (keV) | (dof) | ||||
| 0109141401 | 0.10(1) | 0.99(4) | –0.16(1) | 5.16(5) | 6.42(8) | 2.8(1) | 0.78(3) | 0.29(8) | 2.1(1) | 0.95 (1976) |
| 0157560101 | 0.11(3) | 0.54(1) | –0.34(2) | 0.99(2) | 6.59(7) | 0.9(3) | 0.74(5) | 0.26(1) | 2.7(3) | 0.76 (1976) |
| 0606320101 | 0.09(1) | 0.62(2) | –0.49(2) | 2.47(5) | 6.46(6) | 1.1(2) | 0.75(4) | 0.30(5) | 1.3(2) | 0.87 (1976) |
| 0606320201 | 0.10(1) | 0.73(2) | –0.54(3) | 4.10(7) | 6.59(8) | 2.7(1) | 0.76(3) | 0.32(1) | 1.4(1) | 0.69 (1976) |
| 0606320301 | 0.10(2) | 0.72(2) | –0.49(1) | 4.7(1) | 6.51(4) | 2.5(4) | 0.77(2) | 0.35(4) | 1.6(3) | 0.96 (1976) |
| 0606320401 | 0.10(1) | 0.23(1) | –0.14(6) | 0.74(8) | 6.59(7) | 0.7(3) | 0.78(7) | 0.34(2) | 0.9(4) | 0.72 (2157) |
| 0606321301 | 0.10(3) | 0.87(3) | –0.51(2) | 5.38(9) | 6.41(5) | 3.2(2) | 0.74(5) | 0.33(1) | 2.3(2) | 0.85 (2157) |
| 0606321401 | 0.10(2) | 0.69(4) | –0.54(4) | 4.36(6) | 6.45(4) | 2.6(1) | 0.76(3) | 0.32(5) | 1.5(1) | 0.81 (1976) |
| 0606321501 | 0.10(1) | 0.64(2) | –0.52(3) | 3.59(8) | 6.48(3) | 1.2(1) | 0.77(4) | 0.33(1) | 0.9(4) | 0.74 (1976) |
| 0606321601 | 0.10(1) | 0.93(7) | –0.43(1) | 6.74(8) | 6.39(7) | 3.4(3) | 0.73(5) | 0.35(2) | 3.0(3) | 0.85 (1976) |
| 0606321701 | 0.09(2) | 0.40(2) | –0.49(4) | 1.61(4) | 6.59(8) | 0.9(2) | 0.78(3) | 0.34(4) | 2.2(1) | 0.73 (1976) |
| 0606321801 | 0.10(1) | 0.29(1) | –0.45(2) | 1.21(6) | 6.67(4) | 0.7(1) | 0.75(2) | 0.27(5) | 0.9(2) | 0.77 (1976) |
| 0606321901 | 0.10(1) | 0.23(2) | –0.42(2) | 1.09(3) | 6.59(6) | 0.6(3) | 0.78(4) | 0.21(1) | 0.8(3) | 0.78 (1976) |
| 0606322001 | 0.10(1) | 0.35(1) | –0.51(1) | 2.06(5) | 6.44(4) | 1.0(1) | 0.73(5) | 0.35(2) | 1.1(2) | 0.94 (1976) |
| 0606322101 | 0.10(2) | 0.27(2) | –0.53(2) | 0.71(3) | 6.70(7) | 0.8(2) | 0.78(3) | 0.18(5) | 0.7(1) | 0.83 (1976) |
| 0606322201 | 0.10(1) | 0.32(1) | –0.49(1) | 1.90(4) | 6.59(3) | 1.1(3) | 0.78(4) | 0.23(2) | 1.8(2) | 0.95 (1976) |
| 0606322301 | 0.11(2) | 0.33(2) | –0.54(2) | 1.09(8) | 6.58(7) | 1.0(4) | 0.76(5) | 0.20(1) | 0.9(1) | 0.74 (2157) |
Notes. (a) The spectral model is gabs x (BMC + Laor + redge). (b)Normalization parameters of the BMC and Laor components are in units of 
erg s−1 kpc−2, where L35 is the source luminosity in units of 1035 erg s−2, d10 is the distance to the source in units of 10 kpc, and the Laor and redge components are in units of 10−4 × total photons cm−2 s−1 in line.
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