Observational properties of extreme supernovae

Abstract

The past ten years have opened up a new parameter space in time-domain astronomy with the discovery of transients defying our understanding of how stars explode. These extremes of the transient paradigm represent the brightest—called superluminous supernovae—and the fastest—known as fast blue optical transients—of the transient zoo. The number discovered and information gained per event have witnessed an exponential growth that has benefited observational and theoretical studies. The collected data and the understanding of such events have surpassed any initial expectation and opened up a future exploding with potential, spanning from novel tools of high-redshift cosmological investigation to new insights into the final stages of massive stars. Here, the observational properties of extreme supernovae are reviewed and put in the context of their physics, possible progenitor scenarios and explosion mechanisms.

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Fig. 1: The transient parameter space with peak luminosity as a function of the rise time.
Fig. 2: Prototypical lightcurve evolution of SLSNe I and II.
Fig. 3: Spectroscopic evolution of the three SLSN classes.
Fig. 4: Lightcurve evolution of known rapidly evolving transients (or FBOTs).
Fig. 5: Blue, featureless spectra of fast transients (FBOTs).

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Acknowledgements

The author thanks D. Perley, S. Prentice and M. Pursiainen for sharing their dataset on fast blue optical transients.

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Correspondence to C. Inserra.

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