SIMBAD references

Further to IAUC 8173, M. Hamuy, N. Morrell, J. Arias, and R. Barba report that a spectrum (range 390-900 nm) of SN 2003go (cf. IAUC 8168), obtained on July 30.30 UT with the Baade telescope, shows it to be a type-IIn supernova with a blue continuum and strong Balmer lines in emission, at a redshift of 0.051. Superimposed, narrow, absorption-line components can be seen blueshifted by about 600 km/s from the emission line cores of the Balmer lines. A weak He I 587.6-nm emission is also present.