CAREER: Galactic Archeology: Understanding the Building Blocks of the Milky Way across Cosmic Time

职业:银河考古学:了解宇宙时间银河系的组成部分

基本信息

  • 批准号:
    2045928
  • 负责人:
  • 金额:
    $ 80.01万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Continuing Grant
  • 财政年份:
    2021
  • 资助国家:
    美国
  • 起止时间:
    2021-09-01 至 2026-08-31
  • 项目状态:
    未结题

项目摘要

Dr. Wetzel and his student research team are working to understand how galaxies like our Milky Way (MW) formed. Through this analysis they will they gain an in-depth understanding of the basic building blocks that formed the MW. Catalogs derived from the simulations will be made available to help optimize observational surveys of the MW. The team will develop and disseminate their interactive GalaxyLab program and use it to teach an undergraduate computational astrophysics class.The team will use cosmological simulations to track the population of stars formed in giant molecular clouds (GMCs) in the MW disk and compare it to stars stripped from companion dwarf galaxies. This project builds on the Latte suite of cosmological simulations, which uses the Feedback in Realistic Environments (FIRE) physics model. The new simulations will have a large dynamic range and will resolve GMCs and ultra-faint satellite dwarf galaxies. The team will investigate (1) the origin of the alpha-element bimodality in the abundance distribution of MW stars, (2) the lifetimes, dynamical evolution, and elemental abundances of GMCs and their stellar associations, and (3) "chemical tagging," where the 3D formation history of the MW is reconstructed from trends observed in the distribution of stellar elemental abundances. GalaxyLab will be distributed as a series of modules in an open-source Jupyter Python notebook.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
Wetzel博士和他的学生研究团队正在努力了解像我们银河系(MW)这样的星系是如何形成的。通过这一分析,他们将深入了解构成MW的基本构件。从模拟得出的星表将被提供,以帮助优化对微波辐射的观测调查。该团队将开发和传播他们的互动GalaxyLab程序,并将其用于教授本科生计算天体物理学课程。该团队将使用宇宙学模拟来跟踪在兆瓦圆盘中形成的巨型分子云(GMC)中的恒星数量,并将其与从伴生矮星系中剥离的恒星进行比较。这个项目建立在Latte宇宙学模拟套件的基础上,该套件使用现实环境中的反馈(FIRE)物理模型。新的模拟将有一个大的动态范围,并将解析GMC和超微弱的卫星矮星系。该团队将调查(1)兆瓦恒星丰度分布中阿尔法元素双峰的起源,(2)GMC及其恒星组合的寿命、动力学演化和元素丰度,以及(3)“化学标记”,即根据观测到的恒星元素丰度分布的趋势重建兆瓦恒星的3D形成历史。GalaxyLab将作为一系列模块在开源的Jupyter Python笔记本中分发。该奖项反映了NSF的法定使命,并已通过使用基金会的智力优势和更广泛的影响审查标准进行评估,被认为值得支持。

项目成果

期刊论文数量(26)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
Great balls of FIRE – I. The formation of star clusters across cosmic time in a Milky Way-mass galaxy
巨大的火球 — I. 银河系质量星系中跨越宇宙时间的星团形成
  • DOI:
    10.1093/mnras/stac3573
  • 发表时间:
    2022
  • 期刊:
  • 影响因子:
    4.8
  • 作者:
    Grudić, Michael Y.;Hafen, Zachary;Rodriguez, Carl L.;Guszejnov, Dávid;Lamberts, Astrid;Wetzel, Andrew;Boylan-Kolchin, Michael;Faucher-Giguère, Claude-André
  • 通讯作者:
    Faucher-Giguère, Claude-André
Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation
  • DOI:
    10.3847/1538-4365/acb99a
  • 发表时间:
    2022-02
  • 期刊:
  • 影响因子:
    0
  • 作者:
    A. Wetzel;C. Hayward;R. Sanderson;Xiangcheng Ma;D. Anglés-Alcázar;R. Feldmann;T. K. Chan;K. El-Badry;Coral Wheeler;S. Garrison-Kimmel;F. Nikakhtar;N. Panithanpaisal;Arpit Arora;Alex Gurvich;J. Samuel;Omid Sameie;V. Pandya;Zachary Hafen;C. Hummels;S. Loebman;M. Boylan-Kolchin;J. Bullock;C. Faucher-Giguère;D. Keres̆;E. Quataert;P. Hopkins
  • 通讯作者:
    A. Wetzel;C. Hayward;R. Sanderson;Xiangcheng Ma;D. Anglés-Alcázar;R. Feldmann;T. K. Chan;K. El-Badry;Coral Wheeler;S. Garrison-Kimmel;F. Nikakhtar;N. Panithanpaisal;Arpit Arora;Alex Gurvich;J. Samuel;Omid Sameie;V. Pandya;Zachary Hafen;C. Hummels;S. Loebman;M. Boylan-Kolchin;J. Bullock;C. Faucher-Giguère;D. Keres̆;E. Quataert;P. Hopkins
Born this way: thin disc, thick disc, and isotropic spheroid formation in FIRE-2 Milky Way–mass galaxy simulations
  • DOI:
    10.1093/mnras/stad1806
  • 发表时间:
    2022-10
  • 期刊:
  • 影响因子:
    4.8
  • 作者:
    Sijie Yu;J. Bullock;Alex Gurvich;Zachary Hafen;J. Stern;M. Boylan-Kolchin;C. Faucher-Giguère;
  • 通讯作者:
    Sijie Yu;J. Bullock;Alex Gurvich;Zachary Hafen;J. Stern;M. Boylan-Kolchin;C. Faucher-Giguère;
Reading the CARDs: The Imprint of Accretion History in the Chemical Abundances of the Milky Way's Stellar Halo
  • DOI:
    10.3847/1538-4357/ac78ea
  • 发表时间:
    2021-10
  • 期刊:
  • 影响因子:
    0
  • 作者:
    E. Cunningham;R. Sanderson;K. Johnston;N. Panithanpaisal;M. Ness;A. Wetzel;S. Loebman;I. Escala;D. Horta;C. Faucher-Giguère
  • 通讯作者:
    E. Cunningham;R. Sanderson;K. Johnston;N. Panithanpaisal;M. Ness;A. Wetzel;S. Loebman;I. Escala;D. Horta;C. Faucher-Giguère
On the Stability of Tidal Streams in Action Space
论作用空间潮汐流的稳定性
  • DOI:
    10.3847/1538-4357/ac93fb
  • 发表时间:
    2022
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Arora, Arpit;Sanderson, Robyn E.;Panithanpaisal, Nondh;Cunningham, Emily C.;Wetzel, Andrew;Garavito-Camargo, Nicolás
  • 通讯作者:
    Garavito-Camargo, Nicolás
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Andrew Wetzel其他文献

Gemini observations of galaxies in rich early environments (GOGREEN) I: survey description
双子座对丰富早期环境中星系的观测(GOGREEN)I:调查描述
  • DOI:
    10.1093/mnras/stx1370
  • 发表时间:
    2017
  • 期刊:
  • 影响因子:
    4.8
  • 作者:
    M. Balogh;D. Gilbank;A. Muzzin;G. Rudnick;M. Cooper;C. Lidman;A. Biviano;R. Demarco;S. McGee;J. Nantais;A. Noble;L. Old;G. Wilson;H. Yee;C. Bellhouse;C. Bellhouse;P. Cerulo;J. Chan;I. Pintos;R. Simpson;R. Burg;D. Zaritsky;F. Ziparo;M. V. Alonso;R. Bower;G. Lucia;A. Finoguenov;A. Finoguenov;D. Lambas;H. Muriel;L. Parker;A. Rettura;C. Valotto;Andrew Wetzel;Andrew Wetzel;Andrew Wetzel
  • 通讯作者:
    Andrew Wetzel
The JWST Resolved Stellar Populations Early Release Science Program. V. DOLPHOT Stellar Photometry for NIRCam and NIRISS
詹姆斯韦伯太空望远镜解决了恒星种群早期发布的科学计划。
  • DOI:
  • 发表时间:
    2024
  • 期刊:
  • 影响因子:
    8.7
  • 作者:
    D. Weisz;A. Dolphin;A. Savino;K. McQuinn;M. J. B. Newman;Benjamin F. Williams;N. Kallivayalil;Jay Anderson;Martha L. Boyer;M. Correnti;M. Geha;Karin M. Sandstrom;A. Cole;J. Warfield;E. Skillman;R. E. Cohen;R. Beaton;A. Bressan;A. Bolatto;M. Boylan;Alyson Brooks;James S Bullock;Charlie Conroy;Michael C. Cooper;Julianne J. Dalcanton;A. Dotter;Tobias K. Fritz;C. Garling;M. Gennaro;K. Gilbert;Léo Girardi;Benjamin D. Johnson;L. C. Johnson;J. Kalirai;Evan N. Kirby;Dustin Lang;P. Marigo;H. Richstein;E. Schlafly;E. Tollerud;Andrew Wetzel
  • 通讯作者:
    Andrew Wetzel

Andrew Wetzel的其他文献

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{{ truncateString('Andrew Wetzel', 18)}}的其他基金

Collaborative Research: Magellanic dwarfs as a key laboratory for dwarf galaxy formation
合作研究:麦哲伦矮星作为矮星系形成的重点实验室
  • 批准号:
    2107772
  • 财政年份:
    2021
  • 资助金额:
    $ 80.01万
  • 项目类别:
    Continuing Grant

相似海外基金

How galactic mergers and their stellar survivors shaped our Milky Way
星系合并及其恒星幸存者如何塑造我们的银河系
  • 批准号:
    DE240100150
  • 财政年份:
    2024
  • 资助金额:
    $ 80.01万
  • 项目类别:
    Discovery Early Career Researcher Award
Galactic Outflows: Pushing the Distance Frontiers
银河流出:推动距离边界
  • 批准号:
    DE240100136
  • 财政年份:
    2024
  • 资助金额:
    $ 80.01万
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    Discovery Early Career Researcher Award
Shedding light on dark matter with galactic dynamics in the Milky Way and beyond
通过银河系及其他星系的星系动力学揭示暗物质
  • 批准号:
    MR/X033740/1
  • 财政年份:
    2024
  • 资助金额:
    $ 80.01万
  • 项目类别:
    Fellowship
Collaborative Research: Using New Ice Cores from Dome C to Test the Assumption of a Constant Galactic Cosmic Ray Flux and Improve Understanding of the Holocene Methane Budget
合作研究:利用 Dome C 的新冰芯测试银河系宇宙射线通量恒定的假设并提高对全新世甲烷收支的理解
  • 批准号:
    2146132
  • 财政年份:
    2023
  • 资助金额:
    $ 80.01万
  • 项目类别:
    Standard Grant
Collaborative Research: Using New Ice Cores from Dome C to Test the Assumption of a Constant Galactic Cosmic Ray Flux and Improve Understanding of the Holocene Methane Budget
合作研究:利用 Dome C 的新冰芯测试银河系宇宙射线通量恒定的假设并提高对全新世甲烷收支的理解
  • 批准号:
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    Standard Grant
The Time Variability and Duty Cycle of Active Galactic Nuclei During Quenching
淬火过程中活动星系核的时间变化和占空比
  • 批准号:
    2307375
  • 财政年份:
    2023
  • 资助金额:
    $ 80.01万
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Postdoctoral Fellowship: MPS-Ascend: Probing small galactic scales in large volumes with the Rubin Observatory
博士后奖学金:MPS-Ascend:利用鲁宾天文台探测大量的小星系尺度
  • 批准号:
    2316748
  • 财政年份:
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Using galactic bar dynamics to probe the nature of dark matter
利用银河棒动力学探测暗物质的性质
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  • 资助金额:
    $ 80.01万
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Indirect search of MeV-scale dark matter by observation of galactic diffuse MeV gamma-rays
通过观测银河系弥散MeV伽马射线间接寻找MeV级暗物质
  • 批准号:
    23H05435
  • 财政年份:
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Collaborative Research: Discriminating Between Galactic Feedback Models with Next Generation Observations
合作研究:区分银河反馈模型与下一代观测
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