TeV Studies of Supernovae Powered Regions using Advanced Shower Analysis Techniques with the VERITAS Gamma-Ray Observatory

使用 VERITAS 伽马射线天文台先进的簇射分析技术对超新星驱动区域进行 TeV 研究

基本信息

  • 批准号:
    1206534
  • 负责人:
  • 金额:
    $ 47.46万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Continuing Grant
  • 财政年份:
    2012
  • 资助国家:
    美国
  • 起止时间:
    2012-07-01 至 2016-06-30
  • 项目状态:
    已结题

项目摘要

Intellectual Merit VERITAS is currently the most sensitive VHE gamma-ray observatory in the world. Operating at the basecamp of the Fred Lawrence Whipple Observatory in Arizona, the VERITAS project expands the Imaging Atmospheric Cherenkov Telescope technique pioneered by its precursor, the Whipple 10m Telescope, to include an array of four 12m telescopes with a multitelescope trigger for an order-of-magnitude improved sensitivity over the previous generation. VERITAS probes the extreme physics of sources such as the jets of Active Galactic Nuclei, Supernovae Remnants, and microquasars and provides an important complement to the Fermi Gamma-ray Space Telescope. This award will provide support for the VERITAS science and collaboration service efforts of the Adler Planetarium & Astronomy Museum researchers. The Adler group will lead the development and optimization of advanced gamma-ray analysis methods to increase the performance of VERITAS and play a leading role in calibration efforts. The Adler's science efforts will utilize the improved array performance in the study of extended supernova remnants and pulsar wind nebulae focusing on the case of the Crab Nebula, particularly in light of the recent discovery of the rapid bright synchrotron flares detected by Fermi. Broader Impact The Adler serves as the lead institution for VERITAS Education and Outreach efforts. Beyond the management aspects of the VERITAS EPO effort, the Adler VERITAS scientists will engage in a variety of efforts including hosting undergraduate interns from collaborating VERITAS institutions, participating in the daily 'Astronomy Conversations' held at the Adler Planetarium's Space Visualization Laboratory, investigating the feasibility of a Citizen Science project to distinguish gamma rays from cosmic rays, and providing planetarium expertise to the VERITAS project office to develop a VERITAS-themed show.
VERITAS是目前世界上最灵敏的甚高能伽马射线观测站。VERITAS项目在亚利桑那州弗雷德·劳伦斯维普莱天文台的大本营运行,它扩展了由其前身维普莱10米望远镜开创的成像大气切伦科夫望远镜技术,包括一个由四个12米望远镜组成的阵列,该望远镜具有多望远镜触发器,灵敏度比上一代提高了一个数量级。VERITAS探测活动星系核、超新星遗迹和微类星体等源的极端物理学,并为费米伽马射线太空望远镜提供重要补充。 该奖项将为阿德勒天文馆天文博物馆研究人员的VERITAS科学和协作服务工作提供支持。Adler团队将领导先进伽马射线分析方法的开发和优化,以提高VERITAS的性能,并在校准工作中发挥主导作用。阿德勒的科学工作将利用改进的阵列性能,研究扩展的超新星遗迹和脉冲星风星云,重点是蟹状星云的情况,特别是鉴于费米探测到的快速明亮的同步加速器耀斑的最新发现。更广泛的影响阿德勒作为领导机构的VERITAS教育和推广工作。除了VERITAS EPO工作的管理方面,阿德勒VERITAS科学家将从事各种工作,包括接待来自VERITAS合作机构的本科实习生,参加在阿德勒天文馆空间可视化实验室举行的每日“天文学对话”,调查公民科学项目的可行性,以区分伽马射线和宇宙射线,并为VERITAS项目办公室提供天文馆专业知识,以开发VERITAS主题展览。

项目成果

期刊论文数量(0)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)

数据更新时间:{{ journalArticles.updateTime }}

{{ item.title }}
{{ item.translation_title }}
  • DOI:
    {{ item.doi }}
  • 发表时间:
    {{ item.publish_year }}
  • 期刊:
  • 影响因子:
    {{ item.factor }}
  • 作者:
    {{ item.authors }}
  • 通讯作者:
    {{ item.author }}

数据更新时间:{{ journalArticles.updateTime }}

{{ item.title }}
  • 作者:
    {{ item.author }}

数据更新时间:{{ monograph.updateTime }}

{{ item.title }}
  • 作者:
    {{ item.author }}

数据更新时间:{{ sciAawards.updateTime }}

{{ item.title }}
  • 作者:
    {{ item.author }}

数据更新时间:{{ conferencePapers.updateTime }}

{{ item.title }}
  • 作者:
    {{ item.author }}

数据更新时间:{{ patent.updateTime }}

Geza Gyuk其他文献

Monitoring, trends and impacts of light pollution
光污染的监测、趋势和影响
  • DOI:
    10.1038/s43017-024-00555-9
  • 发表时间:
    2024-05-23
  • 期刊:
  • 影响因子:
    71.500
  • 作者:
    Hector Linares Arroyo;Angela Abascal;Tobias Degen;Martin Aubé;Brian R. Espey;Geza Gyuk;Franz Hölker;Andreas Jechow;Monika Kuffer;Alejandro Sánchez de Miguel;Alexandre Simoneau;Ken Walczak;Christopher C. M. Kyba
  • 通讯作者:
    Christopher C. M. Kyba

Geza Gyuk的其他文献

{{ item.title }}
{{ item.translation_title }}
  • DOI:
    {{ item.doi }}
  • 发表时间:
    {{ item.publish_year }}
  • 期刊:
  • 影响因子:
    {{ item.factor }}
  • 作者:
    {{ item.authors }}
  • 通讯作者:
    {{ item.author }}

{{ truncateString('Geza Gyuk', 18)}}的其他基金

CDI-Type II: Zooniverse - Conquering the Data Flood with a Transformative Partnership between Citizen Scientists and Machines
CDI-Type II:Zooniverse - 通过公民科学家和机器之间的变革性伙伴关系征服数据洪流
  • 批准号:
    0941610
  • 财政年份:
    2010
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Standard Grant
TeV Studies of Active Galactic Nuclei and Starburst Galaxies with the VERITAS Gamma-ray Observatory
使用 VERITAS 伽马射线天文台对活动星系核和星暴星系进行 TeV 研究
  • 批准号:
    0900928
  • 财政年份:
    2009
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Standard Grant
Pointing Monitor System for the VERITAS Gamma-ray Observatory and TeV Studies of Active Galactic Nuclei
用于 VERITAS 伽马射线天文台和活动星系核 TeV 研究的指向监测系统
  • 批准号:
    0653627
  • 财政年份:
    2007
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Continuing Grant
MPS Internships in Public Science Education - MPS-IPSE: Adler Public Education Fellowships
MPS 公共科学教育实习 - MPS-IPSE:阿德勒公共教育奖学金
  • 批准号:
    0120987
  • 财政年份:
    2001
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Standard Grant

相似海外基金

Advanced Astronomical Instrumentation and Observational Studies of Early Supernovae, Optical Transients and Dwarf Galaxies
先进的天文仪器和早期超新星、光学瞬变和矮星系的观测研究
  • 批准号:
    RGPIN-2019-06524
  • 财政年份:
    2022
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
Advanced Astronomical Instrumentation and Observational Studies of Early Supernovae, Optical Transients and Dwarf Galaxies
先进的天文仪器和早期超新星、光学瞬变和矮星系的观测研究
  • 批准号:
    RGPIN-2019-06524
  • 财政年份:
    2021
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
Toward understanding progenitors and explosion physics of core-collapse supernovae by mutual studies between observations and numerical simulations
通过观测和数值模拟之间的相互研究来了解核心塌陷超新星的前身和爆炸物理
  • 批准号:
    21H01121
  • 财政年份:
    2021
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Grant-in-Aid for Scientific Research (B)
Advanced Astronomical Instrumentation and Observational Studies of Early Supernovae, Optical Transients and Dwarf Galaxies
先进的天文仪器和早期超新星、光学瞬变和矮星系的观测研究
  • 批准号:
    RGPIN-2019-06524
  • 财政年份:
    2020
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
Advanced Astronomical Instrumentation and Observational Studies of Early Supernovae, Optical Transients and Dwarf Galaxies
先进的天文仪器和早期超新星、光学瞬变和矮星系的观测研究
  • 批准号:
    RGPIN-2019-06524
  • 财政年份:
    2019
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
Advanced Astronomical Instrumentation and Observational Studies of Supernovae and Remnants
先进的天文仪器和超新星和遗迹的观测研究
  • 批准号:
    RGPIN-2014-05075
  • 财政年份:
    2018
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
Studies on Superluminous Supernovae: Explosion Mechanisms and Connection to First Supernovae in the Universe
超光度超新星研究:爆炸机制以及与宇宙中第一颗超新星的联系
  • 批准号:
    17K05382
  • 财政年份:
    2017
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Grant-in-Aid for Scientific Research (C)
Advanced Astronomical Instrumentation and Observational Studies of Supernovae and Remnants
先进的天文仪器和超新星和遗迹的观测研究
  • 批准号:
    RGPIN-2014-05075
  • 财政年份:
    2017
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
Advanced Astronomical Instrumentation and Observational Studies of Supernovae and Remnants
先进的天文仪器和超新星和遗迹的观测研究
  • 批准号:
    RGPIN-2014-05075
  • 财政年份:
    2016
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
Advanced Astronomical Instrumentation and Observational Studies of Supernovae and Remnants
先进的天文仪器和超新星和遗迹的观测研究
  • 批准号:
    RGPIN-2014-05075
  • 财政年份:
    2015
  • 资助金额:
    $ 47.46万
  • 项目类别:
    Discovery Grants Program - Individual
{{ showInfoDetail.title }}

作者:{{ showInfoDetail.author }}

知道了