SIMBAD references

H. Maehara, Kwasan Observatory, Kyoto University, reports that a low-resolution spectrogram (range 400-800 nm) of the possible nova reported on CBET 2140 was obtained on Jan. 23.887 UT with the 25-cm telescope of the Kwasan Observatory. The spectrum shows H_alpha, H_beta, and Fe II emission lines. These features suggest that this object is a "Fe II"-class nova. The spectrum has been posted at the following website URL: http://www.kwasan.kyoto-u.ac.jp/~maehara/novae/SGRnova2010_20100123.png