Results of spectral fitting of source 2XMM J104608.7-594306. We show the two pn spectra and folded best-fit models, with residuals. Top: simple absorbed blackbody. Bottom: best-fit neutron star atmosphere at d ~ 2 kpc (B = 10¹² G, T_eff ~ 10⁶ K, N_H = 2.6 × 10²¹ cm^-2). Two Gaussian lines in absorption are added to the model (with energies around 0.55 keV and 1.35 keV).