SIMBAD references

G. H. Marion, Harvard-Smithsonian Center for Astrophysics (CfA), on behalf of the CfA Supernova Group, reports on spectroscopic observations (range 340-740 nm) of 2010hh (cf. CBET 2435) obtained on Sept. 3 UT by P. Berlind with the F. L. Whipple Observatory 1.5-m telescope (+ FAST). Cross-correlation with a library of supernova spectra using the "Supernova Identification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024) shows that the best fit for the spectrum of 2010hh is to that of the sub-luminous (1991bg-like) type-Ia supernova 1986G near maximum light.