Subaru/HDS spectra of V5669 Sgr

We identified three blueshifted absorption systems in our spectra. The first two, referred to as low- and high-velocity components, were noticeably identified among HI Balmer, NaI D, and FeII whose lower energies of transients are low (<4eV).

The third absorption component was identified among NII, HeI, and CII lines whose lower energy levels are relatively high (9-21eV). The absorption lines of ^7^BeII at 3130.583{AA} and 3132.228{AA} were identified as the first and second components in our observations. No evidence suggested the existence of LiI at 6708{AA} in any velocity components.