SIMBAD references

Hiroyuki Maehara, Kwasan Observatory, Kyoto University, reports that a low-resolution spectrum (range 400-800 nm) of this object (cf. CBET 2128) was obtained on Jan. 22.890 UT with the 25-cm telescope at the Kwasan Observatory. The spectrum shows H_alpha and Fe II emission lines and suggests that this object is a classical nova just after maximum. Maehara also writes that CCD images of the nova obtained with a 25-cm telescope at the Kwasan Observatory yield the following magnitudes: Jan. 16.875, I_c = 7.92; 16.875, R_c = 8.37; 16.876, V = 8.77; 16.877, B = 9.54.