SIMBAD references

H. Maehara, Kwasan Observatory, Kyoto University, reports that a low- resolution spectrogram (range 400-800 nm) of the variable was taken on Apr. 29.704 UT with a 25-cm telescope at Kwasan Observatory. The spectrum shows H_alpha and H_beta emission lines with a FWMH of 4000 km/s. The spectrum has been posted at the following website URL: http://www.kwasan.kyoto-u.ac.jp/~maehara/novae/SCOnova2010no2_20100429.png. These features suggest that the object is a classical nova. CCD images obtained with a 25-cm telescope at Kwasan Observatory yield the following magnitudes: Apr. 29.680, I_c = 8.77; 29.681, R_c = 9.45; 29.683, V = 11.21; 29.685, B = 12.03.