{"title":"An Overview of the Insight-HXMT Scientific Satellite Measuring Fundamental Parameters of Black Holes","authors":"Wang Wei, Zhu Hai-fan","doi":"10.1016/j.chinastron.2025.11.006","DOIUrl":null,"url":null,"abstract":"<div><div>This paper systematically reviews the primary methods for measuring the fundamental parameters of black holes — mass and spin, and briefly introduces techniques for determining the distances to black hole binary systems. Through case studies, it highlights the importance of precise distance measurements in refining the fundamental parameters of black holes. This paper explores three common approaches to black hole mass measurement: dynamical methods, spectral fitting, and quasiperiodic oscillations, while discussing their practical applications and inherent limitations based on observational results. In the aspect of spin measurement, the focus is on the research achievements of the <em>Insight</em>-HXMT (Insight Hard X-ray Modulation Telescope) satellite. The paper provides an in-depth analysis of two methods: thermal continuum fitting and reflection component fitting, emphasizing the crucial role of the <em>Insight</em>-HXMT satellite in spin research. It meticulously dissects the theoretical foundations and model assumptions of these two methods and presents their measurement processes through examples. Furthermore, we showcase the role and advantages of the <em>Insight</em>-HXMT satellite in spin measurement using these methods.</div></div>","PeriodicalId":35730,"journal":{"name":"Chinese Astronomy and Astrophysics","volume":"49 4","pages":"Pages 678-701"},"PeriodicalIF":0.0000,"publicationDate":"2025-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy and Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0275106225001079","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2025/12/8 0:00:00","PubModel":"Epub","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0
Abstract
This paper systematically reviews the primary methods for measuring the fundamental parameters of black holes — mass and spin, and briefly introduces techniques for determining the distances to black hole binary systems. Through case studies, it highlights the importance of precise distance measurements in refining the fundamental parameters of black holes. This paper explores three common approaches to black hole mass measurement: dynamical methods, spectral fitting, and quasiperiodic oscillations, while discussing their practical applications and inherent limitations based on observational results. In the aspect of spin measurement, the focus is on the research achievements of the Insight-HXMT (Insight Hard X-ray Modulation Telescope) satellite. The paper provides an in-depth analysis of two methods: thermal continuum fitting and reflection component fitting, emphasizing the crucial role of the Insight-HXMT satellite in spin research. It meticulously dissects the theoretical foundations and model assumptions of these two methods and presents their measurement processes through examples. Furthermore, we showcase the role and advantages of the Insight-HXMT satellite in spin measurement using these methods.
本文系统地回顾了测量黑洞基本参数质量和自旋的主要方法,并简要介绍了确定黑洞双星距离的技术。通过案例研究,强调了精确的距离测量在提炼黑洞基本参数中的重要性。本文探讨了三种常用的黑洞质量测量方法:动力学方法、光谱拟合方法和准周期振荡方法,并根据观测结果讨论了它们的实际应用和固有局限性。在自旋测量方面,重点介绍了Insight- hxmt (Insight Hard x射线调制望远镜)卫星的研究成果。深入分析了热连续体拟合和反射分量拟合两种方法,强调了Insight-HXMT卫星在自旋研究中的关键作用。详细剖析了这两种方法的理论基础和模型假设,并通过实例介绍了它们的测量过程。此外,我们还展示了Insight-HXMT卫星在使用这些方法进行自旋测量中的作用和优势。
期刊介绍:
The vigorous growth of astronomical and astrophysical science in China led to an increase in papers on astrophysics which Acta Astronomica Sinica could no longer absorb. Translations of papers from two new journals the Chinese Journal of Space Science and Acta Astrophysica Sinica are added to the translation of Acta Astronomica Sinica to form the new journal Chinese Astronomy and Astrophysics. Chinese Astronomy and Astrophysics brings English translations of notable articles to astronomers and astrophysicists outside China.