The Astrophysical Journal (Jan 2023)

VERITAS and Fermi-LAT Constraints on the Gamma-Ray Emission from Superluminous Supernovae SN2015bn and SN2017egm

  • A. Acharyya,
  • C. B. Adams,
  • P. Bangale,
  • W. Benbow,
  • J. H. Buckley,
  • M. Capasso,
  • V. V. Dwarkadas,
  • M. Errando,
  • A. Falcone,
  • Q. Feng,
  • J. P. Finley,
  • G. M. Foote,
  • L. Fortson,
  • A. Furniss,
  • G. Gallagher,
  • A. Gent,
  • W. F Hanlon,
  • O. Hervet,
  • J. Holder,
  • T. B. Humensky,
  • W. Jin,
  • P. Kaaret,
  • M. Kertzman,
  • M. Kherlakian,
  • D. Kieda,
  • T. K Kleiner,
  • S. Kumar,
  • M. J. Lang,
  • M. Lundy,
  • G. Maier,
  • C. E McGrath,
  • J. Millis,
  • P. Moriarty,
  • R. Mukherjee,
  • M. Nievas-Rosillo,
  • S. O’Brien,
  • R. A. Ong,
  • S. R. Patel,
  • K. Pfrang,
  • M. Pohl,
  • E. Pueschel,
  • J. Quinn,
  • K. Ragan,
  • P. T. Reynolds,
  • D. Ribeiro,
  • E. Roache,
  • J. L. Ryan,
  • I. Sadeh,
  • M. Santander,
  • G. H. Sembroski,
  • R. Shang,
  • M. Splettstoesser,
  • D. Tak,
  • J. V. Tucci,
  • A. Weinstein,
  • D. A. Williams,
  • VERITAS collaboration,
  • B. D. Metzger,
  • M. Nicholl,
  • I. Vurm

DOI
https://doi.org/10.3847/1538-4357/acb7e6
Journal volume & issue
Vol. 945, no. 1
p. 30

Abstract

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Superluminous supernovae (SLSNe) are a rare class of stellar explosions with luminosities ∼ 10–100 times greater than ordinary core-collapse supernovae. One popular model to explain the enhanced optical output of hydrogen-poor (Type I) SLSNe invokes energy injection from a rapidly spinning magnetar. A prediction in this case is that high-energy gamma-rays, generated in the wind nebula of the magnetar, could escape through the expanding supernova ejecta at late times (months or more after optical peak). This paper presents a search for gamma-ray emission in the broad energy band from 100 MeV to 30 TeV from two Type I SLSNe, SN2015bn, and SN2017egm, using observations from Fermi-LAT and VERITAS. Although no gamma-ray emission was detected from either source, the derived upper limits approach the putative magnetar’s spin-down luminosity. Prospects are explored for detecting very-high-energy (VHE; 100 GeV–100 TeV) emission from SLSNe-I with existing and planned facilities such as VERITAS and CTA.

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