Wide-field optical transient surveys collectively discover ∼50 new transients per night, making rapid, multi-filter and/or spectroscopic follow-up of all but the most exceptional events unfeasible. Consequently, the (early) light-curve properties of most supernovae (SNe), particularly sub-luminous events, are often poo...
O. Mogawana, P. Groot, N. Blagorodnova et al.· Publications of the Astronom...· 0 citations
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