SIMBAD references

D. Steeghs, Harvard-Smithsonian Center for Astrophysics, reports on optical spectroscopy of XTE J1814-338 (cf. IAUC 8144) on June 22.2 UT with the 6.5-m Magellan/Clay telescope (+ Boller & Chivens spectrograph) at Las Campanas: "Prominent hydrogen and helium emission lines were detected in the spectrum of the optical- counterpart candidate reported by Krauss et al. (IAUC 8154). The classic hallmarks of an interacting binary spectrum firmly establishes the optical counterpart of the accreting pulsar. The strongest spectral feature was double-peaked H_alpha emission with FWHM = 800 km/s and equivalent width 0.6 nm."