Multi-epoch X-ray observations of SLSN-I 2018bsz support ejecta-CSM interaction as the dominant X-ray powering mechanism rather than a central magnetar.
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Fermi-LAT detection of GeV emission from SN 2017egm favors a magnetar central engine over CSM interaction for powering this superluminous supernova.
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Multi-Epoch X-Ray Detection of SLSN-I 2018bsz: Constraints on the Powering Mechanism and Ejecta Structure
Multi-epoch X-ray observations of SLSN-I 2018bsz support ejecta-CSM interaction as the dominant X-ray powering mechanism rather than a central magnetar.
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Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine
Fermi-LAT detection of GeV emission from SN 2017egm favors a magnetar central engine over CSM interaction for powering this superluminous supernova.