SIMBAD references

G. H. Marion and P. Challis, Harvard-Smithsonian Center for Astrophysics (CfA), on behalf of the CfA Supernova Group, report on spectroscopic observations (range 340-740 nm) of 2010hk (cf. CBET 2439) obtained on Sept. 4 UT by P. Berlind and of 2010ho (cf. CBET 2445) on Sept. 5 UT by M. Calkins 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 both 2010hk and 2010ho are normal type-Ia supernovae at a few days past maximum light.