SN 2022ann: a Type Icn Supernova from a Dwarf Galaxy That Reveals Helium in Its Circumstellar Environment
K. W. Davis,K. Taggart,S. Tinyanont,R. J. Foley,V. A. Villar,L. Izzo,C. R. Angus,M. J. Bustamante-Rosell,D. A. Coulter,N. Earl,D. Farias,J. Hjorth,M. E. Huber,D. O. Jones,P. L. Kelly,C. D. Kilpatrick,D. Langeroodi,H-Y Miao,C. M. Pellegrino,E. Ramirez-Ruiz,C. L. Ransome,S. Rest,M. R. Siebert,G. Terreran, I. M. Thornton,S. K. Yadavalli,G. R. Zeimann,K. Auchettl,C. R. Bom,T. G. Brink,J. Burke,Y. Camacho-Neves,K. C. Chambers,T. J. L. de Boer,L. DeMarchi,A. V. Filippenko,L. Galbany,C. Gall,H. Gao,F. R. Herpich,D. A. Howell,W. V. Jacobson-Galan,S. W. Jha,A. Kanaan,N. Khetan,L. A. Kwok, Z. Lai,C. Larison,C-C Lin, K. C. Loertscher,E. A. Magnier,C. McCully,P. McGill,M. Newsome,E. Padilla Gonzalez,Y-C Pan,A. Rest,J. Rho,T. Ribeiro,A. Santos,W. Schoenell, S. N. Sharief,K. W. Smith,R. J. Wainscoat,Q. Wang,Y. Zenati,W. Zheng MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY（2023）
Key words
stars: massive,binaries,transients: supernovae
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