SIMBAD references

P. Challis and R. P. Kirshner, Harvard-Smithsonian Center for Astrophysics; and P. Garnavich, University of Notre Dame, report that a spectrum (range 350-730 nm) of V466 And was obtained with the 1.5-m Tillinghast telescope (+ FAST spectrograph) on Sept. 3.497 UT, showing a strong blue continuum with H_alpha and H_beta in emission. Later Balmer lines are a combination of broad absorption and weak emission. The FWHM of H_alpha is 600 km/s. Also seen are He I 492.1-, 587.5-, 667.8-, 501.5-, and 706.5-nm and He II 486.1-nm. The spectrum is that of a dwarf nova in outburst.