Table 3: Best-fit parameters of the power-law plus four Gaussians model reproducing the [18-20] Å  RGS-1 spectra of Mkn 421. The error bars refer to the 90% confidence intervals.
RGS-1 [18-20] Å
Feature $\lambda$ FWHM k
number (Å) (mÅ) ( cts cm-2 s-1 Å-1)
ToO observation
2 $18.661\pm0.004$ $\rm 24^{+9}_{-6}$ $-0.0040\pm0.0011$
3 $18.937\pm0.001$ $8\pm1$ $0.0111\pm0.0023$
5 $19.662\pm0.005$ $30\pm10$ $-0.0040\pm0.0010$
6 $19.890\pm0.001$ $\rm 8.5^{+1.5}_{-1}$ $-0.0098\pm0.0031$
Archival data
2 $18.683\pm0.001$ $\rm 15.2^{+3}_{-2}$ $-0.319\pm0.048$
3 $18.9585\pm0.001$ $14.5\pm2$ $-0.349\pm0.051$
5 $19.681\pm0.002$ $15\pm3$ $-0.266\pm0.053$
6 $19.910\pm0.002$ $16\pm3$ $-0.303\pm0.050$
Total
2 $18.680\pm0.004$ $\rm 33^{+9}_{-7}$ $-0.147\pm0.026$
3 $18.953\pm0.003$ $\rm 28^{+5}_{-4}$ $-0.177\pm0.029$
5 $19.676\pm0.003$ $\rm 23^{+5}_{-4}$ $-0.166\pm0.032$
6 $19.904\pm0.004$ $\rm 33^{+8}_{-7}$ $-0.128\pm0.027$


Source LaTeX | All tables | In the text