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The Hydrogen-Poor Superluminous Supernovae from the Zwicky Transient Facility Phase-I Survey: I. Data

Z. H. Chen,Lin Yan Y. H. Yao, O. Yaron

semanticscholar(2022)

Cited 0|Views2
Abstract
Z. H. Chen, Lin Yan, T. Kangas, R. Lunnan, S. Schulze, J. Sollerman, D. A. Perley, T.-W. Chen, A. Gal-Yam, X. F. Wang, 8 I. Andreoni, E. Bellm, J. S. Bloom, 12 K. Burdge, A. Burgos, D. Cook, A. Dahiwale, K. De, R. Dekany, A. Dugas, S. Frederik, C. Fremling, M. Graham, M. Hankins, A. Ho, J. Jencson, V. Karambelkar, M. Kasliwal, S. Kulkarni, R. Laher, B. Rusholme, Y. Sharma, F. Taddia, K. Taggart, L. Tartaglia, A. Tzanidakis, J. Van Roestel, R. Walter, Y. Yang, Y. H. Yao, and O. Yaron
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要点】:本文研究了来自Zwicky Transient Facility Phase-I Survey的氢贫超亮超新星,揭示了其特性和演化过程,为理解这类特殊天体提供了新见解。

方法】:作者利用Zwicky Transient Facility (ZTF) 的数据,结合其他天文观测设施的数据,对氢贫超亮超新星进行分类和分析。

实验】:通过ZTF Phase-I Survey收集的数据,对发现的超新星样本进行观测分析,使用的数据集名称为ZTF数据集,实验结果显示了氢贫超亮超新星的光学特性和光谱特征。