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Home All issues Volume 505 / No 1 (October I 2009) A&A, 505 1 (2009) 417-439 Full HTML
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Table 4:

Spectral fit results for combined JEM-X and IBIS/ISGRI data.
Name JEM-X $N_{\rm H}^b$ $f_{3-20~\rm keV}^c$ $f_{20-100~\rm keV}^c$ $\Gamma $ $E_{\rm C}$ $\log L_{3 - 100~\rm keV}$ $\chi^2_\nu$(d.o.f.)
  $[\sigma]$ $[10^{22}~\rm cm^{-2}]$       $[\rm keV]$ $[\rm erg~s^{-1}]$  
1ES 0033+59.5 10.1 0.36 6.0 1.4 $2.75 {+0.18 \atop -0.16}$ - 45.16 0.51 (8)
NGC 1275a 38.6 3.75 22.8 3.0 - - 43.58 >5a
3C 120 5.5 0.2 5.8 7.5 $1.76 \pm 0.06$ - 44.52 0.67 (15)
Mrk 421 155.7 0.08 61.6 32.5 $2.12 {+0.05 \atop -0.04}$ $133 {+32 \atop -21}$ 45.29 1.43 (14)
NGC 4151a 91.5 6.9 33.2 40.4 $1.75 {+0.04 \atop -0.06}$ $170 {+30 \atop -32}$ 43.25 1.36 (14)
NGC 4388a 14.3 27 10.3 26.0 $1.26 {+0.15 \atop -0.16}$ $78 {+35 \atop -20}$ 43.68 0.41 (15)
NGC 4593 a 7.0 0.02 4.4 7.7 $1.46 {+0.07 \atop -0.15}$ $193 {+12 \atop -93}$ 43.34 1.01 (15)
Cen Aa 57.2 12.5 28.1 43.4 $1.85 \pm 0.01$ - 42.94 1.49 (17)
MCG-06-30-015 11.2 0.03 7.0 5.0 $2.10 \pm 0.05$ - 42.93 0.79 (10)
4U 1344-60a 8.3 5 5.6 21.0 $1.47 {+0.11 \atop -0.16}$ $86 {+31 \atop -22}$ 43.70 0.76 (15)
IC 4329Aa 11.3 0.42 14.5 21.1 $1.41 \pm 0.08$ $86 {+18 \atop -13}$ 44.31 1.29 (15)
Circinus Galaxya 5.3 360 3.9 21.0 $1.2 \pm 0.2$ $30 \pm 3$ 42.03 1.52 (11)
NGC 5506 16.8 3.4 12.1 8.0 $2.20 \pm 0.08$ - 43.27 0.66 (12)
H 1426+428 7.5 <0.02 6.1 1.2 $2.83 {+0.25 \atop -0.21}$ - 44.90 0.67 (9)
Mrk 501 7.9 0.013 10.2 4.8 $2.3 \pm 0.1$ - 44.60 0.73 (15)
GRS 1734-292a 10.5 3.7 6.7 8.0 $1.25 {+0.10 \atop -0.16}$ $39 {+5 \atop -6}$ 44.02 1.28 (12)
IGR J17488-3253a 21.8 0.72 1.7 2.9 $1.63 \pm 0.03$ - 43.11 1.10 (119)
QSO B1957+405a 10.5 20 16.2 8.3 $1.9 {+0.1 \atop -0.2}$ - 45.26 0.76 (9)
Mrk 509 7.2 <0.01 7.5 9.3 $1.8 \pm 0.1$ - 44.66 0.69 (8)
IGR J21178+5139 17.1 2 1.5 2.2 $1.7 \pm 0.1$ - - 1.61 (13)
IGR J21247+5058a 54.1 0.6 9.5 11.1 $1.4 \pm 0.1$ $61 {+22 \atop -11}$ 44.27 1.41 (11)
3C 454.3 6.4 0.5 10.7 20.3 $1.54 \pm 0.05$ - 47.93 0.58 (16)
1H 2251-179 10.7 <0.19 5.7 7.2 $1.8 \pm 0.1$ - 45.10 1.20 (13)

a see Appendix A; b $N_{\rm H}$ values have been fixed during the fit; c fluxes are given in $[10^{-11}~\rm erg~cm^{-2}~s^{-1}]$


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