SIMBAD references

H. Naito and N. Tokimasa, Nishi-Harima Astronomical Observatory (NHAO); and H. Yamaoka, Kyushu University, report: "A low-resolution spectrum (range 400-850 nm, resolution 150) of the possible nova reported on IAUC 8483, obtained on Feb. 11.8 UT with the NHAO 0.60-m telescope, shows prominent and broad Balmer lines in emission, which suggests that it is indeed a classical nova. The FWHM of the H_alpha line is 3200 km/s. The nearest object in the Digitized Sky Survey images is a star (mag about 18) located 2".5 west-southwest of the reported position."