SIMBAD references

R. B. Perry, Langley Research Center, NASA; R. J. Rudy, D. K. Lynch, T. R. Prater, S. Mazuk, and A. M. Gilbert, The Aerospace Corporation; and R. C. Puetter, University of California, San Diego; report 0.47- to 2.5-micron spectroscopy of V2467 Cyg (cf. IAUC 8821, 8888) on 2007 Dec. 14 UT using VNIRIS on the Lick 3-m telescope. The object remains bright and shows many high- excitation emission lines. Coronal lines of [SI VII], [Ca VIII], [Si X], and [S XI] showed notched, doubled line profiles. Also present were lines of H I, He I, He II, weak O I, and the unidentified novae lines. There was no evidence of thermal emission from dust.