利用 CSST 预测超新星观测结果: I. 测光样本

IF 6.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY
Chengqi Liu, Youhua Xu, Xianmin Meng, Xin Zhang, Shi-Yu Li, Yuming Fu, Xiaofeng Wang, Shufei Liu, Zun Luo, Guanghuan Wang, Hu Zhan
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引用次数: 0

摘要

中国空间站望远镜(CSST,又称 "讯天")是一台可使用的两米口径宽视场望远镜,与中国空间站在同一轨道上运行。中国空间站计划对银河系中高纬度 17,500 德2 的天空区域进行勘测,深度为 25-26 AB 等,至少有 6 个光度波段,波长在 255-1,000 纳米之间。在如此大的天空区域内,还将在与成像巡天相同的波长范围内拍摄无缝光谱。尽管 CSST 巡天不是专门进行时域研究的,但它仍将探测到大量的瞬变星,如超新星(SNe)。在本文中,我们使用 Sncosmo 软件包模拟了基于草图巡天计划的测光 SN 观测。在为期 10 年的巡天期间,CSST 预计将观测到约 500 万个各种类型的 SNe。通过质量削减,我们获得了一个 "黄金 "样本,其中包括大约 7,400 个 SNe Ia、2,200 个 SNe Ibc 和 6,500 个 SNe II 候选者,其正确分类率分别达到 91%、63% 和 93%(正式定义为分类精度)。同样的巡天还能触发警报,在光最大值出现前至少两天探测到约 15500 个 SNe Ia(精确度为 61%)和 2100 个 SNe II(精确度为 49%)候选天体。此外,CSST 的近紫外观测每年还能偶然捕捉到数百个震荡冷却事件。这些结果表明,CSST 可以为 SN 研究做出潜在的重大贡献。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Forecasting supernova observations with the CSST: I. Photometric samples

The China Space Station Telescope (CSST, also known as Xuntian) is a serviceable two-meter-aperture wide-field telescope operating in the same orbit as the China Space Station. The CSST plans to survey a sky area of 17,500 deg2 of the medium-to-high Galactic latitude to a depth of 25–26 AB mag in at least 6 photometric bands over 255–1,000 nm. Within such a large sky area, slitless spectra will also be taken over the same wavelength range as the imaging survey. Even though the CSST survey is not dedicated to time-domain studies, it would still detect a large number of transients, such as supernovae (SNe). In this paper, we simulate photometric SN observations based on a strawman survey plan using the Sncosmo package. During its 10-year survey, the CSST is expected to observe about 5 million SNe of various types. With quality cuts, we obtain a “gold” sample that comprises roughly 7,400 SNe Ia, 2,200 SNe Ibc, and 6,500 SNe II candidates with correctly classified percentages reaching 91%, 63%, and 93% (formally defined as classification precision), respectively. The same survey can also trigger alerts for the detection of about 15,500 SNe Ia (precision 61%) and 2,100 SNe II (precision 49%) candidates at least two days before the light maxima. Moreover, the near-ultraviolet observations of the CSST will be able to catch hundreds of shock-cooling events serendipitously every year. These results demonstrate that the CSST can make a potentially significant contribution to SN studies.

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来源期刊
Science China Physics, Mechanics & Astronomy
Science China Physics, Mechanics & Astronomy PHYSICS, MULTIDISCIPLINARY-
CiteScore
10.30
自引率
6.20%
发文量
4047
审稿时长
3 months
期刊介绍: Science China Physics, Mechanics & Astronomy, an academic journal cosponsored by the Chinese Academy of Sciences and the National Natural Science Foundation of China, and published by Science China Press, is committed to publishing high-quality, original results in both basic and applied research. Science China Physics, Mechanics & Astronomy, is published in both print and electronic forms. It is indexed by Science Citation Index. Categories of articles: Reviews summarize representative results and achievements in a particular topic or an area, comment on the current state of research, and advise on the research directions. The author’s own opinion and related discussion is requested. Research papers report on important original results in all areas of physics, mechanics and astronomy. Brief reports present short reports in a timely manner of the latest important results.
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