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机译:Ia型超新星后期近红外光曲线中的一年平稳
Ctr Astrophys Harvard & Smithsonian Cambridge MA 02138 USA|Amer Museum Nat Hist Dept Astrophys New York NY 10024 USA;
Trinity Coll Dublin Sch Phys Dublin Ireland;
Space Telescope Sci Inst 3700 San Martin Dr Baltimore MD 21218 USA;
Univ Edinburgh Inst Astron Edinburgh Midlothian Scotland|Univ Birmingham Birmingham Inst Gravitat Wave Astron Birmingham W Midlands England|Univ Birmingham Sch Phys & Astron Birmingham W Midlands England;
Ctr Astrophys Harvard & Smithsonian Cambridge MA 02138 USA;
Space Telescope Sci Inst 3700 San Martin Dr Baltimore MD 21218 USA|Johns Hopkins Univ Dept Phys & Astron Baltimore MD 21218 USA;
Queens Univ Belfast Sch Math & Phys Astrophys Res Ctr Belfast Antrim North Ireland;
Univ New South Wales Australian Def Force Acad Sch Sci Canberra ACT Australia;
Univ Massachusetts Dartmouth Dept Phys N Dartmouth MA USA;
机译:ASASSN-14lp的后期观测加强了Ia型超新星的峰值光度与它们的后期光曲线形状之间的相关性
机译:CFAIR2:94型Ia超新星的近红外光曲线
机译:Ia型超新星的近红外光曲线
机译:Supernovae II型的V波段轻曲线形态
机译:爆炸条件在Ia型超新星后期光谱上的印记
机译:利用LightCycler实时PCR和荧光共振能量转移杂交探针熔解曲线分析快速鉴定百日咳百日咳杆菌毒素基因变异。
机译:ASASSN-14LP的后期观察加强了IA型超新型峰值亮度与其后期光曲线形状之间的相关性的情况