Dear all, The spectrum of Nova Sgr 2001 taken at Bisei Astronomical Observatory on Feb. 25.88 UT, which we reported in [vsnet-alert 5723] (and IAUC 7589), can be seen at http://vsnet.town.bisei.okayama.jp/bao/astro/nova/nova_sgr_2001.gif In addition to emission lines reported earlier, Fe II lines are evident. There are 'shoulders' on the profile of H-alpha and H-beta lines. There may be P-Cyg absorption troughs blueward of H-alpha and H-beta. Best regards, Kazuya Ayani