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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,B. D. Metzger,M. Nicholl,I Vurm

The Astrophysical Journal（2023）

Cited 1|Views65
Key words
Shocks,Gamma-rays,Particle astrophysics,Supernovae,Magnetars,Millisecond pulsars
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