基本信息
张岚 女 硕导 中国科学院国家天文台
电子邮件: zhanglan@bao.ac.cn
通信地址: 北京市朝阳区大屯路甲20号
邮政编码:
电子邮件: zhanglan@bao.ac.cn
通信地址: 北京市朝阳区大屯路甲20号
邮政编码:
招生信息
招生专业
070401-天体物理
招生方向
银河系结构与演化
教育背景
2006-09--2012-06 中科院国家天文台 博士2002-09--2006-06 南京大学 理论物理学士
工作经历
工作简历
2020-07~现在, 中科院国家天文台, 副研究员2016-10~2020-06,中科院国家天文台, 助理研究员2014-10~2016-09,智利大学天文系, 博士后2012-09~2014-09,中科院国家天文台, 助理研究员2006-09~2012-06,中科院国家天文台, 博士2002-09~2006-06,南京大学, 理论物理学士
出版信息
发表论文
(1) Preliminary Exploration of Areal Density of Angular Momentum for Spiral Galaxies, Preliminary Exploration of Areal Density of Angular Momentum for Spiral Galaxies, RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2023, 第 1 作者(2) A Catalog of Distance Determinations for the LAMOST DR8 K Giants in the Galactic Halo, THE ASTRONOMICAL JOURNAL, 2023, 第 1 作者(3) Exploring the Galactic Anticenter Substructure with LAMOST and Gaia DR2, ASTROPHYSICAL JOURNAL, 2021, 第 11 作者(4) The mass of the Milky Way out to 100 kpc using halo stars, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 第 11 作者(5) Effects of satellite lines in fittings of He-like triplets of X-ray Spectra, Proceedings of the International Astronomical Union, 2020, 第 1 作者(6) Measuring the local dark matter density with LAMOST DR5 and Gaia DR2, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 第 6 作者(7) Tracing Kinematic and Chemical Properties of Sagittarius Stream by K-Giants, M-Giants, and BHB stars, ASTROPHYSICAL JOURNAL, 2019, 第 7 作者(8) Identifying Galactic Halo Substructure in 6D Phase Space Using similar to 13,000 LAMOST K Giants, ASTROPHYSICAL JOURNAL, 2019, 第 4 作者(9) The Origins of Young Stars in the Direction of the Leading Arm of the Magellanic Stream: Abundances, Kinematics, and Orbits *, ASTROPHYSICAL JOURNAL, 2019, 第 1 作者 通讯作者(10) A wide star-black-hole binary system from radial-velocity measurements, NATURE, 2019, 第 27 作者(11) A New Hyper-runaway Star Discovered from LAMOST and Gaia: Ejected Almost in the Galactic Rotation Direction, ASTRONOMICAL JOURNAL, 2018, 第 9 作者(12) The mass of the Galactic dark matter halo from similar to 9000 LAMOST DR5 K giants, RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2018, 第 3 作者(13) The mass of the Galactic dark matter halo from -9000 LAMOST DR5 K giants, The mass of the Galactic dark matter halo from -9000 LAMOST DR5 K giants, 天文和天体物理学研究:英文版, 2018, 第 3 作者(14) Physical parameter estimation with MCMC from observations of Vela X-1, HIGH POWER LASER SCIENCE AND ENGINEERING, 2018, 第 1 作者(15) Chemical Composition of Young Stars in the Leading Arm of the Magellanic System, ASTROPHYSICAL JOURNAL, 2017, 第 1 作者 通讯作者(16) NGC 1980 Is Not a Foreground Population of Orion: Spectroscopic Survey of Young Stars with Low Extinction in Orion, ASTRONOMICAL JOURNAL, 2017, 第 5 作者(17) Determining the local dark matter density with LAMOST data, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 第 5 作者(18) THE GRAVITATIONAL POTENTIAL NEAR THE SUN FROM SEGUE K-DWARF KINEMATICS, ASTROPHYSICAL JOURNAL, 2013, 第 1 作者 通讯作者(19) The identification of comets in Chinese historical records, SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2011, 第 1 作者(20) CHEMICAL COMPOSITIONS OF KINEMATICALLY SELECTED OUTER HALO STARS, ASTROPHYSICAL JOURNAL, 2009, 第 1 作者 通讯作者
科研活动
科研项目
( 1 ) 中国科学院稳定支持基础研究领域 青年团队计划, 参与, 中国科学院计划, 2022-07--2027-06
参与会议
(1)Physical parameter estimation with MCMC from X-ray observations 2019-04-14