SIMBAD references

A. Arai, T. Kajikawa, C. Naka, Kyoto Sangyo University, write that their low-resolution spectroscopy on Sept. 7.42 UT using the Araki telescope at Koyama Astronomical Observatory suggest that the object is an "Fe II"-type classical nova, highly reddened by the interstellar medium. F. Walter, Stony Brook University; and J. Seron, Cerro Tololo Interamerican Observatory (CTIO), confirm that V1313 Sco is a young galactic nova from a spectrum obtained on Sept. 8.091 with the SMARTS/CTIO 1.5-m reflector (range 565-695 nm), with broad H_alpha emission having a triple-peaked spectrum that is reminiscent of early recurrent-novae spectra. Further observational details are given on CBET 2813.