Nova Sgr 2002 (No. 3): spectroscopic confirmation by Mitsugu Fujii Mitsugu Fujii (Fujii Bisei Observatory, Okayama, Japan) reports (via K. Ayani, Bisei Astronomical Observatory) the spectrum of Haseda's new object taken on 2002 Sep. 21.44 UT. The object shows strong Balmer and Fe II emission lines. The FWHM of Halpha emission is 2400 km/s. This observation confirms that the object is an Fe II-class nova shortly after maximum. Regards, Taichi Kato