SIMBAD references

L. Tomasella, S. Valenti, A. Pastorello, M. Fiaschi, anD S. Benetti, Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Padova, on behalf of a larger collaboration, report that a low-S/N spectrogram of 2011hl was obtained on Oct. 30.87 UT with the Ekar-Copernico 1.82-m telescope (+ AFOSC; range 380-820 nm; resolution 2.2 nm). Cross-correlation with a library of supernova spectra using the "Supernova Identification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024) suggests that 2011hl is a type-Ia supernova at z = 0.08, two months after maximum.