Key points are not available for this paper at this time.
Superluminous supernovae (SLSNe) are a new class of transients with luminosities 10 -100 times larger than the usual core-collapse supernovae (SNe). Their origin is still unclear and one widely discussed scenario involves a millisecond magnetar central engine. The GeV-TeV emission of SLSNe has been predicted in the literature but has not been convincingly detected yet. Here we report the search for the -ray emission in the direction of SN 2017egm, one of the closest SLSNe detected so far, with the 15-year Fermi-LAT Pass 8 data. There is a transient -ray source appearing about 2 months after this event and lasting a few months. Both the peak time and the luminosity of the GeV emission are consistent with the magnetar model prediction, suggesting that such a GeV transient is the high-energy counterpart of SN 2017egm and the central engine of this SLSNe is a young magnetar.
Shang et al. (Mon,) studied this question.