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  1. No Access

    Article

    Observation of inverse Compton emission from a long γ-ray burst

    Long-duration γ-ray bursts (GRBs) originate from ultra-relativistic jets launched from the collapsing cores of dying massive stars. They are characterized by an initial phase of bright and highly variable radi...

    P. Veres, P. N. Bhat, M. S. Briggs, W. H. Cleveland, R. Hamburg, C. M. Hui… in Nature (2019)

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    Article

    A kilonova as the electromagnetic counterpart to a gravitational-wave source

    Observations and modelling of an optical transient counterpart to a gravitational-wave event and γ-ray burst reveal that neutron-star mergers produce gravitational waves and radioactively powered kilonovae, an...

    S. J. Smartt, T.-W. Chen, A. Jerkstrand, M. Coughlin, E. Kankare, S. A. Sim… in Nature (2017)

  3. Article

    Correction: Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions

    Nature 502, 346–349 (2013); doi:10.1038/nature12569 In this Letter, we have identified an important error affecting Fig. 4 and Extended Data Fig. 6, as well as the values of some parameters derived from our mo...

    M. Nicholl, S. J. Smartt, A. Jerkstrand, C. Inserra, M. McCrum, R. Kotak… in Nature (2016)

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    Article

    Slowly fading super-luminous supernovae that are not pair-instability explosions

    Observations of two slow-to-fade super-luminous supernovae are reported; both show relatively fast rise times and blue colours, which are incompatible with pair-instability models.

    M. Nicholl, S. J. Smartt, A. Jerkstrand, C. Inserra, M. McCrum, R. Kotak… in Nature (2013)