SIMBAD references

D. K. Lynch, R. W. Russell, D. Kim, The Aerospace Corporation; and M. L. Sitko and S. Brafford, University of Cincinnati and Space Science Institute, report that 3- to 13-micron spectroscopy of V2362 Cyg (cf. IAUC 8731) on Dec. 12.25 UT using BASS on the Infrared Telescope Facility showed a smooth stellar-like continuum decreasing monotonically toward longer wavelengths between 3 and 13 microns with no evidence of thermal emission from dust. Infrared magnitudes at that time were L = 5.0 ± 0.1, M = 4.5 ± 0.2, N = 4.0 ± 0.2.