SIMBAD references

Filippenko and Chornock add that inspection of CCD spectra, obtained as above on Nov. 29 UT, reveals that SN 2003ih (IAUC 8207) is of type Ib/Ic, 2 ± 1 months past maximum brightness; the near- infrared Ca II triplet emission is especially strong. SN 2003ki (IAUC 8245) is of type IIb, about 3-4 weeks after the explosion; weak He I absorption lines are present in the spectrum, whose hydrogen Balmer lines exhibit P-Cyg profiles. The redshift of its host galaxy is 0.025, measured from narrow emission lines in an H II region.