Self-consistent Stellar Radial Velocities from LAMOST Medium-Resolution Survey (MRS) DR7
Self-consistent Stellar Radial Velocities from LAMOST Medium-Resolution Survey (MRS) DR7
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Author / Creator
Zhang, Bo , Jiao, Li , Yang, Fan , Jian-Ping Xiong , Jian-Ning Fu , Liu, Chao , Tian, Hao , Yin-Bi, Li , Jia-Xin, Wang , Cai-Xia, Liang , Yu-Tao, Zhou , Wei-kai Zong , Cheng-Qun Yang , Liu, Nian and Yong-Hui, Hou
Publisher
Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Radial velocity (RV) is among the most fundamental physical quantities obtainable from stellar spectra and is rather important in the analysis of time-domain phenomena. The LAMOST Medium-Resolution Survey (MRS) DR7 contains 5 million single-exposure stellar spectra at spectral resolution \(R\sim7\,500\). However, the temporal variation of the RV ze...
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Full title
Self-consistent Stellar Radial Velocities from LAMOST Medium-Resolution Survey (MRS) DR7
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TN_cdi_proquest_journals_2532403089
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2532403089
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2105.11624
