Institutional Repository System Of Yunnan Observatories, CAS
The preliminary statistical analysis of LAMOST DR9 low resolution quasi-stellar objects | |
Chen, Y.H.1,2,3; Tang, M.Y.1,2,4; Shu, H.1,2,3 | |
发表期刊 | NEW ASTRONOMY |
2023-07 | |
卷号 | 101 |
DOI | 10.1016/j.newast.2023.102013 |
收录类别 | SCI |
关键词 | QSOs Statistical analysis-QSOs LAMOST DR9-QSOs |
摘要 | Based on more than 10 years of large-scale spectral sky survey, LAMOST DR9 v1.0 low resolution catalog has released 76167 data of QSOs. We adopt 48704 QSOs with redshift Z from 0.0 to 6.0, the error of redshift from 0.0 to 0.06, and the galactic latitude |b| > 30 degrees to do a research work. There are 95.36% of QSOs with the error of redshift less than or equal to 0.025. Therefore, the Z values are very reliable with small errors. Some statistical figures about Z are drawn and preliminarily analyzed. The distribution of QSOs with Z in different directions shows that universe is spatially isotropic in large-scale structure. The QSOs with high Z values and low Z values correspond to the decelerating and accelerating expansion of the universe respectively, the epoch of the matter dominance and the dark energy dominance respectively. In the epoch of matter dominance, the number density of QSOs in the statistical figures is more than that in the epoch of dark energy dominance and the gravity can slow the expansion. The large-scale spectral sky survey is helpful for us to better understand the past, present and future of the universe. |
资助项目 | National Development and Reform Commission, China ; NSFC, China[11803004] |
项目资助者 | National Development and Reform Commission, China ; NSFC, China[11803004] |
语种 | 英语 |
学科领域 | 天文学 ; 恒星与银河系 |
文章类型 | Article |
出版者 | ELSEVIER |
出版地 | RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS |
ISSN | 1384-1076 |
URL | 查看原文 |
WOS记录号 | WOS:000942951200001 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | DIGITAL SKY SURVEY ; 1ST DATA RELEASE ; ACCELERATING UNIVERSE ; SUPERNOVA ; TELESCOPE ; GAIA |
引用统计 | |
文献类型 | 期刊论文 |
版本 | 出版稿 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/25868 |
专题 | 中国科学院天体结构与演化重点实验室 |
通讯作者 | Chen, Y.H. |
作者单位 | 1.Institute of Astrophysics, Chuxiong Normal University, Chuxiong 675000, China; 2.School of Physics and Electronical Science, Chuxiong Normal University, Chuxiong 675000, China; 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, China; 4.Department of Astronomy, Yunnan University, and Key Laboratory of Astroparticle Physics of Yunnan Province, Kunming, 650091, China |
推荐引用方式 GB/T 7714 | Chen, Y.H.,Tang, M.Y.,Shu, H.. The preliminary statistical analysis of LAMOST DR9 low resolution quasi-stellar objects[J]. NEW ASTRONOMY,2023,101. |
APA | Chen, Y.H.,Tang, M.Y.,&Shu, H..(2023).The preliminary statistical analysis of LAMOST DR9 low resolution quasi-stellar objects.NEW ASTRONOMY,101. |
MLA | Chen, Y.H.,et al."The preliminary statistical analysis of LAMOST DR9 low resolution quasi-stellar objects".NEW ASTRONOMY 101(2023). |
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The preliminary stat(1739KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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