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
DOI10.1016/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
ISSN1384-1076
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
被引频次:2[WOS]   [WOS记录]     [WOS相关记录]
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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