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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
Source PublicationNEW ASTRONOMY
2023-07
Volume101
DOI10.1016/j.newast.2023.102013
Indexed BySCI
KeywordQSOs Statistical analysis-QSOs LAMOST DR9-QSOs
Abstract

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.

Funding ProjectNational Development and Reform Commission, China ; NSFC, China[11803004]
Funding OrganizationNational Development and Reform Commission, China ; NSFC, China[11803004]
Language英语
Subject Area天文学 ; 恒星与银河系
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherELSEVIER
Publication PlaceRADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
ISSN1384-1076
URL查看原文
WOS IDWOS:000942951200001
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordDIGITAL SKY SURVEY ; 1ST DATA RELEASE ; ACCELERATING UNIVERSE ; SUPERNOVA ; TELESCOPE ; GAIA
Citation statistics
Document Type期刊论文
Version出版稿
Identifierhttp://ir.ynao.ac.cn/handle/114a53/25868
Collection中国科学院天体结构与演化重点实验室
Corresponding AuthorChen, Y.H.
Affiliation1.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
Recommended Citation
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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