Table 2: Fluxes and iron line properties for the Chandra observations analysed in this paper. The iron line fluxes and EWs refer to the "local'' fits (see text for details).
Source ${F}_{\rm0.5{-}2~keV}$ a ${F}_{\rm 2{-}10~keV}$ a ${\it EW}_{\rm Fe}$ b ${I}_{\rm Fe}$ c
NGC 1386 $\rm 1.8^{+1.5}_{-0.5}$ $2.4\pm1.0$ $\rm 1.5^{+0.8}_{-0.5}$ $\rm0.6^{+0.3}_{-0.2}$
NGC 3393 $\rm 2.2^{+0.5}_{-0.2}$ $2.6\pm0.8$ $0.6\pm0.3$ $0.4\pm0.2$
NGC 5347 $\rm0.27\pm0.06$ $2.4\pm0.7$ $1.7\pm0.7$ $0.5\pm0.2$
NGC 5643 $1.4\pm0.2$ 6.3+2.1-2.0 $\rm 1.5^{+0.8}_{-0.6}$ $\rm 1.3^{+0.7}_{-0.5}$
NGC 7212 $\rm0.8^{+0.1}_{-0.2}$ $\rm 5.2^{+1.3}_{-1.2}$ $0.7\pm0.3$ $0.7\pm0.3$
a In units of 10-13 erg cm-2 s-1; b Iron line EW in units of keV;
c Iron line flux in units of 10-5 ph cm-2 s-1.

Source LaTeX | All tables | In the text