论文标题

本地宇宙I的Zwicky瞬态设施人口普查:对钙富差异瞬变的系统搜索揭示了三个相关的光谱子类

The Zwicky Transient Facility Census of the Local Universe I: Systematic search for Calcium rich gap transients reveal three related spectroscopic sub-classes

论文作者

De, Kishalay, Kasliwal, Mansi M., Tzanidakis, Anastasios, Fremling, U. Christoffer, Adams, Scott, Andreoni, Igor, Bagdasaryan, Ashot, Bellm, Eric C., Bildsten, Lars, Cannella, Christopher, Cook, David O., Delacroix, Alexandre, Drake, Andrew, Duev, Dmitry, Dugas, Alison, Frederick, Sara, Gal-Yam, Avishay, Goldstein, Daniel, Golkhou, V. Zach, Graham, Matthew J., Hale, David, Hankins, Matthew, Helou, George, Ho, Anna Y. Q., Irani, Ido, Jencson, Jacob E., Kaye, Stephen, Kulkarni, S. R., Kupfer, Thomas, Laher, Russ R., Leadbeater, Robin, Lunnan, Ragnhild, Masci, Frank J., Miller, Adam A., Neill, James D., Ofek, Eran O., Perley, Daniel A., Polin, Abigail, Prince, Thomas A., Quataert, Eliot, Reiley, Dan, Riddle, Reed L., Rusholme, Ben, Sharma, Yashvi, Shupe, David L., Sollerman, Jesper, Tartaglia, Leonardo, Walters, Richard, Yan, Lin, Yao, Yuhan

论文摘要

(删节)使用Zwicky瞬态设施警报流,我们正在开展一项大型运动,以对当地宇宙(CLU)目录中普查中的星系中发生的所有瞬变进行光谱分类。实验的目的是构建一个频谱完整的,容量限制的瞬态样本,这些瞬态在100英寸的Clu星系中重合至200 MPC,并深度为20 mag。我们描述了操作的前16个月中的调查设计和光谱完整性。我们从操作的前16个月中完整性。我们从系统搜索量$ pap probients $ peep $ peep $ peep(22个低液体)中的结果(22个较低的液体)(绝对),可绝对<MASBORBY(mosection $),绝对是mosem umin umin umin umin的频率,可绝对<MASBORBY $)。在实验中发现的事件(在754个光谱分类的SNE中,我们报告了八个钙富的缝隙瞬变的检测,并将其体积速率限制为至少$ \ \ \ pm5 $ 15 \ pm5 $ \ pm5 $%。在CA-IB/C事件中,IB/C样特征(CA-IB/C对象)。变形阶段。我们发现,光谱连续性,体积速率和历时一时,与低质量白色矮人的爆炸性燃烧一致他的炮弹或外壳爆炸以低密度的爆炸。

(Abridged) Using the Zwicky Transient Facility alert stream, we are conducting a large campaign to spectroscopically classify all transients occurring in galaxies in the Census of the Local Universe (CLU) catalog. The aim of the experiment is to construct a spectroscopically complete, volume-limited sample of transients coincident within 100" of CLU galaxies out to 200 Mpc, and to a depth of 20 mag. We describe the survey design and spectroscopic completeness from the first 16 months of operations. We present results from a systematic search for Calcium rich gap transients in the sample of 22 low luminosity (peak absolute magnitude $M > -17$), hydrogen poor events found in the experiment (out of 754 spectroscopically classified SNe). We report the detection of eight Calcium rich gap transients, and constrain their volumetric rate to be at least $\approx 15\pm5$% of the SN Ia rate. Combining this sample with ten events from the literature, we find a likely continuum of spectroscopic properties ranging from events with SN Ia-like features (Ca-Ia objects) to SN Ib/c-like features (Ca-Ib/c objects) at peak light. Within the Ca-Ib/c events, we find two populations of events distinguished by their red ($g - r \approx 1.5$ mag) or green ($g - r \approx 0.5$ mag) spectral colors at $r$-band peak, wherein redder events show strong line blanketing signatures, slower light curves, weaker He lines and lower [Ca II]/[O I] in the nebular phase. Together, we find that the spectroscopic continuum, volumetric rates and striking old environments are consistent with the explosive burning of He shells on low mass white dwarfs. We posit that Ca-Ia and red Ca-Ib/c objects are consistent with the double detonation of He shells with high He burning efficiency, while green Ca-Ib/c objects could arise from less efficient He burning scenarios such as detonations in low density He shells or He shell deflagrations.

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