**Table 1:** MP Mus best-fit paramenters.
Par.	best-fit value
T^a	$\rm 2.7^{+0.1}_{-0.2}$	$\rm 7.2^{+0.4}_{-0.5}$	$\rm 36^{+18}_{-11}$
EM^b	$\rm 9.6^{+5.2}_{-2.5}$	$\rm 17.9^{+4.0}_{-3.0}$	$\rm 2.9^{+1.5}_{-0.8}$
$N_{\rm H}^c$	$\rm 4.6^{+1.8}_{-1.7}$
Ab.^d	$\rm O = 0.25^{+0.08}_{-0.07}$	$\rm Ne = 0.76^{+0.23}_{-0.15}$	$\rm S = 0.28\pm0.20$	$\rm Fe = 0.09^{+0.04}_{-0.02}$

^a Temperature (MK). ^b Emission Measure $({\rm 10^{52}~cm^{-3}})$ . ^c Hydrogen column density $({\rm 10^{20}~cm^{-2}})$ . ^d Abundances refer to the solar photospheric values of Asplund et al. (2005). All the uncertainties correspond to the 68% confidence level.

Source LaTeX | All tables | In the text