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Millimeter-wavelength transients and sources with the Atacama Cosmology Telescope and the Simons Observatory

Millimeter-wavelength transients and sources with the Atacama Cosmology Telescope and the Simons Observatory
阿塔卡马宇宙学望远镜和西蒙斯天文台的毫米波瞬变和源
批准号:
2206344
负责人:
Kevin Huffenberger
金额:
$64.78万
依托单位:
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2022
资助国家:
美国
项目状态:
未结题
起止时间:
2022-09-01 至 2025-08-31

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中文摘要
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英文摘要
Precision measurements of the cosmic microwave background radiation seek a clearer picture of the physics of the Big Bang. The telescopes that take such data also capture light from stars and galaxies that emit at the same wavelengths. This project would build software pipelines that take advantage of these measurements. Each day, these telescopes scan the sky and make an updated image, letting sources that are variable to be identified. During this decade, upgraded telescopes will produce more and better data of this kind. Such time-resolved data will permit new classes of unknown phenomena to be found. This may include exceptional supernovae, gamma ray bursts, tidal disruptions of stars around supermassive black holes, stellar flares and the discovery of additional bodies in the solar system, including a hypothetical and undiscovered Planet 9. The excitement of this project will be conveyed to the public via a variety of outreach programs including one targeting people living in rural areas near Tallahassee.New, time-domain studies of wide-field millimeter-wave surveys are opening a vast, unexplored discovery space. In this project, millimeter-wave transients and point-like sources will be identified using data from the Advanced Atacama Cosmology Telescope, now surveying areas that exceed 18,000 square degrees, and the Simons Observatory, which by the mid-2020s will produce more sensitive measurements over a similar area. Software tools and pipelines will be developed to (1) develop and implement a system to mine daily Simons Observatory data based on real-time transient alerts; (2) perform triggered and blind searches for mm-wave transients in archival and live data; (3) prepare and release point source catalogs in temperature and polarization for the ACT and Simons Observatory surveys; and (4) support a follow-up program for high redshift source candidates. The project supports a number of outreach programs that involve the general public, K-12 students and undergraduate as well as graduate students.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.
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CMB Polarization Foreground Effects on B-modes and Lensing
  • 批准号:
    2009870
  • 项目类别:
    Standard Grant
  • 资助金额:
    $53.37万
  • 财政年份:
    2020
  • 负责人:
    Kevin Huffenberger
  • 依托单位:
Next Generation Data Analysis For Next Generation Cosmic Microwave Background Experiments.
  • 批准号:
    1815887
  • 项目类别:
    Standard Grant
  • 资助金额:
    $59.42万
  • 财政年份:
    2018
  • 负责人:
    Kevin Huffenberger
  • 依托单位:
海外基金