Hee-Jong 搜索引擎优化
新闻
教育
- Ph.D. 亚利桑那大学天文学. 2001年秋季至2007年8月
- B.S. 天文学，亚利桑那大学，优等生. 1999年春季至2001年秋季
- B.S. 物理学，亚利桑那大学最优等生. 1999年春季至2001年秋季
- B. 韩国釜山国立大学药学专业. 1990年春季至1994年春季
专业的会员
- 暗能量光谱仪器 (DESI), Co-Chair of the Galaxy Quasar Clustering Science Working Group for DESI, Feb 2017-Present
- 斯隆数字巡天 (SDSS IV) - eBOSS(扩展重子振荡光谱调查), eBOSS的平铺协调员, SDSS-IV建筑师.
- 天体物理研究所 (ApI)
研究兴趣
宇宙学、星系调查;
- Baryon acoustic oscillations and redshift-space distortions from galaxy redshift surveys
- 来自宇宙剪切的大尺度群集
- Mitigation of observational systematics in galaxy surveys using deep learning methods
- 重子声学振荡从21cm强度映射.
My research interests are in high precision 宇宙学 with large scale structure. I study the distributions of 星系 and matter on very large scales to infer how our Universe has expanded, 我们的宇宙是由什么组成的, and therefore to collect observational clues to identify dark energy and dark matter, 它们加在一起构成了宇宙的95%，但仍然很神秘.
The main topics of my work involve the detection of the Baryon Acoustic Oscillations (BAO) from the large scale structure of 星系 and matter. 这一特征很早就形成了, hot Universe by the sound waves propagated in the plasma of photons and baryons due to the interaction between photon pressure and gravity. The propagating sound waves have been frozen near the epoch of so called 'Recombination' when the baryons and photons are effectively separated.
The current distribution of 星系 and matter still trace the imprint of this primordial sound saves on very large scales. The true size of this feature is known quite accurately; therefore, 通过比较观察到的尺寸和已知的真实尺寸, 我们可以估计到各个宇宙时代的距离. This relation of distance to cosmic epoch encodes the expansion history of the Universe and therefore the properties of dark energy that drives the expansion faster and faster.
这个特征的巨大尺寸(~0.50亿光年)需要非常大的星系调查, such as Baryon Oscillations Spectroscopic Survey (BOSS) which has been completed, 最近发表了一系列论文(http://sdss3.org//science/boss_publications.php), 正在进行的eBOSS(扩展BOSS) , 暗能量光谱仪器(DESI)将于2018年启动.
我一直在积极参与所有这些任务.
以及BAO特性, these surveys also intend to study the large scale streams of the 星系 (i.e, 星系 move around) to study the nature of Gravity, dark matter, and dark energy. My work involves various methods of analyzing the large scale structure of 星系 and matter, 包括分析, 数值, 观察性研究, 作为一个暗能量探测器. I am also interested in relating observed 星系 to the underlying dark matter halo distributions, 利用大尺度结构寻找中微子质量的上限, 暗物质分布的弱引力透镜信号.
协同活动
- DESI Y1 BAO重点项目联合召集人，2020年2月-至今
- Co-Chair of the Galaxy Quasar Clustering Science Working Group for DESI, Feb 2017- Mar 2020
- 欧洲研究理事会:启动资助小组，同行评审小组，2020年
- SDSS-IV架构师，2015.07 -
- Tiling coordinator for the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), July 2013-2019
- 开发一个公开的BAO预测代码与教授. 丹尼尔·爱森斯坦，2007年
选定的出版物
- 搜索引擎优化, 姬钟和*太田, Atsuhisa和Schmittfull, 马塞尔和齐藤, 顺和比特勒, Florian: Iterative reconstruction excursions for Baryon Acoustic Oscillations and beyond, 2022年mnras. 514.3396M
- 缪勒(Eva-Maria)和* Rezaie, Mehdi和Percival, Will J. 罗斯是阿什利·J. (搜索引擎优化, 6th author):The clustering of 星系 in the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Primordial non-Gaussianity in Fourier Space,2022年mnras.514.3396M
- ∗在线旅行社, Atsuhisa和搜索引擎优化, 姬钟和斋藤, 顺和比特勒, Florian : Modeling iterative reconstruction and displacement field in the large scale structure, 物理评论D, 104, 123508, 理论物理. 牧师. D 104, 123508
- * * * * * *. 和搜索引擎优化, 姬钟和穆勒, Eva-Maria : Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey- I: Catalogue preparation and systematic mitigation,2021年mnras.506.3439R
- ∗梅尔兹, 格兰特和雷扎伊, Mehdi和搜索引擎优化,Hee-Jong :The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey quasar sample: testing observational systematics on the Baryon Acoustic Oscillation measurement,2021年mnras.506.2503M
- Zarrouk, Pauline和∗Rezaie, Mehdi和Raichoor, Anand :Baryon acoustic oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric 星系 from the DESI Legacy Imaging Surveys,2021年mnras.503.2562Z
- 杉山，Naonori S. 和斋藤, 顺和比特勒, 弗洛里安和苏, Hee-Jong: Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues, 2021年mnras.501.2862S
- Mohammad, Faizan G. 以及威尔·J·珀西瓦尔. 和搜索引擎优化, Hee-Jong : The completed SDSS-IV extended baryon oscillation spectroscopic survey: pairwise-inverse probability and angular correction for fibre collisions in clustering measurements,2020年mnras.498..128M
- 杉山，Naonori S. 和斋藤, 顺和比特勒, 弗洛里安和苏, Hee-Jong: Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space, 2020年mnras.497.1684S
- A complete FFT-based decomposition formalism for the redshift-space bispectrum. Sugiyama N.~S.斋藤，S.布鲁斯、F., & 搜索引擎优化,H.-J. 2018年,arXiv: 1803.02132
- 未来重子声学振荡调查的理论系统. 叮,Z.徐，H.-J.， Vlah, Z.等。. 中国生物医学工程学报，2018,33 (4):1021
- The clustering of 星系 in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample. 阿拉姆,年代.等。. 中国生物医学工程学报，2017,33 (4):559 - 567
- The clustering of 星系 in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space. 布鲁斯、F.、搜索引擎优化., H.-J.罗斯，A.等。. [j] .中国生物医学工程学报，2017,44 (4):344 - 344
- The clustering of 星系 in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space. 布鲁斯、F.、搜索引擎优化., H.-J.斋藤，S.等。.[j] .中文信息学报，2017,422,2242
- 傅里叶空间重构BAO的建模. 搜索引擎优化,H.-J.布鲁斯、F.罗斯，A.~J.斋藤，S.[j] .中国生物医学工程学报，2016,46 (6):2453
- 前景楔形和21厘米BAO测量. 搜索引擎优化,H.-J. & Hirata C. M.[j] .中文信息学报，2016,45 (6):342
- Improved Forecasts for the Baryon Acoustic Oscillations and Cosmological Distance Scale. 搜索引擎优化,H. -J. & 艾森斯坦,D. J. 2007年4月，第6卷第14页
- Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak. 艾森斯坦,D. J.徐，H.-j.西尔科，E., & Spergel D. 2007, ApJ, 664, 675
- Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys. 搜索引擎优化,H.-J., & 艾森斯坦,D. J. 2003, ApJ, 598, 720
奖助金
- “Improving Dark Energy Constraints Using Low-Redshift Large-Scale Structures,“DE-SC, (PI), 9/1/2022-4/30/2024, 能源部, 科学办公室, 高能物理办公室, $150,000
- BAO的最优鲁棒重构, 红移空间扭曲和阿尔科克-帕钦斯基效应,de-sc0019091 (pi), 9/2018-8/2023, 能源部, 科学办公室, 高能物理办公室, 早期职业奖, $750,000
- “Improving Dark Energy Constraints Using Low Redshift Large Scale Structures,DE-SC0014329 (Co-PI), 4/2018-3/2021, 能源部, 科学办公室, 高能物理办公室, ($335,000)
- “Improving Dark Energy Constraints Using Low Redshift Large Scale Structures,DE-SC0014329 (Co-PI), 4/2017-3/2018, 能源部, 科学办公室, 高能物理办公室, ($140,000)
- “Improving Dark Energy Constraints Using Low Redshift Large Scale Structures,DE-SC0014329 (Co-PI), 7/2015-3/2017, 能源部, 科学办公室, 高能物理办公室, ($240,000)
课程
本科: Introduction to 理论物理ics: you can explain many of the everyday physical phenomena if you take this course *well*, 运动学, 牛顿定律, 圆周运动, 液体, thermodynamics; Fundamentals of Astrophysics: Introduction to celestial Mechanics, 恒星天体物理学, 望远镜, 星系, 宇宙学
本科/研究生: Interstellar Medium and Galaxies: An advanced lecture focusing on 星系 and 宇宙学