Dear colleages, M. Fujii (Amateur astronomer, Okayama, Japan) and H. Kawakita (Amateur astronomer, Osaka, Japan) informed me that they had carried out spectroscopic observation of possible nova in Scopius at June 7.6 UT with a hand-made spectrograph mounted on the 0.28m Schmidt Cassegrain telescope. The width and length of the slit correspond to 7 arcsec and 424 arcsec, respectively, and the spectral resolution was 1.2 nm. Strong and broad emission lines of H-alpha (observed FWHM ~ 3200 km/s) and H-beta were found in their spectra, while the instrumental resolution was 550 km/s. I believe that it is indeed a nova. Best regards, Kazuya Ayani Bisei Astronomical Observatory