SIMBAD references

S. Valenti and S. Benetti, Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Padova, on behalf of a larger collaboration, report that a spectrogram (range 330-750 nm; resolution 1.5 nm) of PSN J01452477-0349353 = SN 2011dp, obtained on June 25.38 UT with the European Southern Observatory's New Technology Telescope (+ EFOSC), is that of a type-Ia supernova. After cross-correlation with a library of supernova spectra via the "GELATO" code (Harutyunyan et al. 2008, A.Ap. 488, 383; available at website URL https://gelato.tng.iac.es/login.cgi), the spectrum of 2011dp appears to be very similar to that of SN 2003du (Stanishev et al. 2007, A.Ap. 469, 645) at 52 days after maximum light.