SIMBAD references

L. Tomasella, A. Pastorello, S. Valenti, and S. Benetti, Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Padova, on behalf of a larger collaboration, report that a spectrogram of 2011he, obtained on Oct. 29.78 UT with the Ekar-Copernico 1.82-m telescope (+ AFOSC; range 360-810 nm; resolution 2.2 nm), suggests that it is a type-Ia supernova at z = 0.05 and several weeks after its B-band maximum brightness. The spectrum shares similarity with those of type-Ia supernovae of the 1991T-like subgroup.