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[1]Wang,S.Q.,Wang,L.J.,Dai,Z.G.,&Wu,X.F.,SuperluminousSupernovaePoweredbyMagnetars:Late-timeLightCurvesandHardEmissionLeakage,TheAstrophysicalJournal,799,107:1-8(2015)
[2]Wang,S.Q.,Wang,L.J.,Dai,Z.G.,&Wu,X.F.,AUnifiedEnergy-reservoirModelContainingContributionsfrom56NiandNeutronStarsandItsImplicationforLuminousTypeIcSupernovae,TheAstrophysicalJournal,807,147:1-10(2015)
[3]Wang,S.Q.,Liu,L.D.,Dai,Z.G.,Wang,L.J.,&Wu,X.F.,ATriple-energy-sourceModelforSuperluminousSupernovaiPTF13ehe,TheAstrophysicalJournal,828,87:1-5(2016)
[4]Wang,S.Q.,Cano,Z.,Wang,L.J.,etal.,ModelingTheMostLuminousSupernovaAssociatedwithaGamma-RayBurst,SN2011kl,TheAstrophysicalJournal,850,148:1-9(2017)
[5]Wang,S.Q.,Cano,Z.,Li,L.,etal.,ModelingtheLightCurvesoftheLuminousTypeIcSupernova2007D,TheAstrophysicalJournal,877,20:1-7(2019)
[6]Li,L.,Wang,S.Q*.,Liu,L.D.,WangX.G.,LiangE.W.,Dai,Z.G.TheEnergySourcesofDouble-peakedsuperluminoussupernovaPS1-12cilandluminoussupernovaSN2012aa,TheAstrophysicalJournal,891,98,pp.1-8,(2020)
[7]Wang,L.J,Wang,S.Q.,Dai,Z.G.,XuD.,Han,Y.H.,Wu,X.F.,&Wei,J.Y.,OpticalTransientsPoweredbyMagnetars:Dynamics,LightCurves,andTransitiontotheNebularPhase,TheAstrophysicalJournal,821,22:1-10(2016)
[8]Dai,Z.G.,Wang,S.Q.,Wang,J.S.,Wang,L.J.,&Yu,Y.W.,TheMostLuminousSupernovaASASSN-15lh:SignatureofaNewbornRapidlyRotatingStrangeQuarkStar,TheAstrophysicalJournal,817,132:1-6(2016)
[9]Liu,L.D.,Wang,S.Q.,Wang,L.J.,Dai,Z.G.,Yu,H.,&Peng,Z.K.,AMonteCarloApproachtoMagnetar-poweredTransients.I.Hydrogen-deficientSuperluminousSupernovae,TheAstrophysicalJournal,842,26:1-11(2017)
[10]Peng,Z.K.,Wang,S.Q.,Liu,L.D.,Dai,Z.G.,Yu,H.ConstrainingtheEnvironmentalPropertiesofFRB131104UsingtheUnifiedDynamicalAfterglowModel,TheAstrophysicalJournal,861,147:1-9(2018)
[11]Wang,L.J.,Cano,Z.,Wang,S.Q.,Zheng,W.,etal.AMonteCarloApproachtoMagnetar-poweredTransients:II.Broad-linedTypeIcSupernovaeNotAssociatedwithGRBs,TheAstrophysicalJournal,851,54:1-16(2017)
[12]Wang,L.J.,Wang,X.F.,Wang,S.Q.,Dai,Z.G.,Liu,L.D.,Song,L.M.,Rui,L.M.,Cano,Z.,&Li,B.,AfallbackaccretionmodelfortheunusualtypeII-PsupernovaiPTF14hls,TheAstrophysicalJournal,TheAstrophysicalJournal,865,95:1-8(2018)
[13]Liu,L.D.,Wang,L.J.,Wang,S.Q.,&Dai,Z.G.,AMultipleEjecta-circumstellarMediumInteractionModelandItsImplicationsforSuperluminousSupernovaeiPTF15esbandiPTF13dcc,TheAstrophysicalJournal,856,59:1-8(2018)
[14]Wang,L.J.,Han,Y.H.,Xu,D.,Wang,S.Q.,Dai,Z.G.,Wu,X.F.,&Wei,J.Y.,Solvingthe56NiPuzzleoftheMagnetar-poweredBroad-linedTypeIcSupernovae,TheAstrophysicalJournal,831,41:1-7(2016)
[15]Wang,L.J.,Yu,H.,Liu,L.D.,Wang,S.Q.,Han,Y.H.,Xu,D.,Dai,Z.G,Qiu,Y.L.,&Wei,J.Y.,EvidenceforMagnetarFormationinbroad-linedTypeIcSupernovae1998bwand2002ap,TheAstrophysicalJournal,837,128:1-7(2017)
[16]Wang,L.J.,Wang,X.F.,Cano,Z.,Wang,S.Q.,Liu,L.D.,Dai,Z.G.,etal.Broad-linedTypeIcSupernovaiPTF16asu:AChallengetoAllExistingModels,MonthlyNoticesoftheRoyalAstronomicalSociety,489,110(2019)
[17]Gangopadhyay,A.,MisraK.,Hiramatsu,D.,Wang,S.Q.,Hosseinzadeh,G.etal.FlashionizationsignaturesinthetypeIbnsupernovaSN2019uo,TheAstrophysicalJournal,889,170,pp.1-14,2020
[18]Wen-JinXie,LeZou,Hong-BangLiu,Shan-QinWang,En-WeiLiang,MagnetarasCentralEngineofGamma-RayBursts:Quasi-UniversalJet,EventRateandX-rayLuminosityFunctionofDipoleRadiation,TheAstrophysicalJournal,inpress,2020
已发表的综述论文（6篇）
[19]Wang,S.Q.,Dai,Z.G.,&Wu,X.F.ResearchDevelopmentsinLi-PaczyńskiNovae(kilonovae)(I):TheoreticalAspect,ChAA,40,2:141-175,2016
[20]Wang,S.Q.,Dai,Z.G.,&Wu,X.F.ResearchDevelopmentsinLi-PaczyńskiNovae(kilonovae)(II):ObservationalAspect,ChAA,40,4:439-473,2016
[21]Wang,S.Q.,Wang,L.J.,&Dai,Z.G.,TheEnergySourcesofSuperluminousSupernovae,InvitedReviewacceptedforpublicationinResearchinAstronomyandAstrophysics,19,63:1-20(2019)
[22]Cano,Z.,Wang,S.Q.,Dai,Z.G.,&Wu,X.F.TheObserver'sGuidetotheGamma-RayBurstSupernovaConnection,AdAst,2017,E5:1-42(2017)
[23]王善钦，戴子高，吴雪峰.《GRB130427A/SN2013cq与伽玛射线暴-超新星成协》,《天文学进展》,32,481(2014)
[24]耿金军，肖笛，王善钦，戴子高，《引力波的电磁对应体》,《中国科学》,48(7),079802,2018
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