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SI2-SSE: Hearing the Signal through the Static: Realtime Noise Reduction in the Hunt for Binary Black Holes and other Gravitational Wave Transients

SI2-SSE: Hearing the Signal through the Static: Realtime Noise Reduction in the Hunt for Binary Black Holes and other Gravitational Wave Transients
SI2-SSE:通过静电听到信号:寻找双黑洞和其他引力波瞬变过程中的实时降噪
批准号:
1642391
负责人:
Chad Hanna
金额:
$40.0万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2016
资助国家:
美国
项目状态:
已结题
起止时间:
2016-11-01 至 2020-10-31

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中文摘要
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英文摘要
Gravitational waves - tiny ripples in the fabric of space - were detected for the first time in history on September 14, 2015 by the US-led gravitational wave observatory, LIGO. This watershed event has ushered in a new era of gravitational wave astronomy, which will transform our understanding of the Universe by providing information through a previously inaccessible channel. LIGO operates at the very edge of the sensitivity required to detect gravitational waves, and therefore, non-stationary noise caused by the environment, e.g., weather and man-made noise, limits LIGO's sensitivity to short-duration gravitational wave transient signals such as the one detected in September. In order to ensure the most opportunity for the advancement of science, this project aims to mine the extensive auxiliary information available in the LIGO observatories in realtime in order to mitigate the impact of non-stationary noise and increase the rate of transient gravitational wave detections. Doing so will afford increased opportunities for joint gravitational wave and electromagnetic observations, which are thought to be rare.This project aims to address a key piece of missing software infrastructure to use machine learning and inference techniques to utilize auxiliary information such as seismometers, microphones and various control loop signals, to identify non-stationary noise that couples to the gravitational-wave channel in near realtime. The software will be broken into three components: a signal decomposer, a signal classifier and a signal trainer. The signal classifier will determine, given the decomposed, instantaneous output of auxiliary channels and the training data, the probability that non-stationary noise is present. These software components will be built from reusable resources that can be applied across the time-domain gravitational wave community in data calibration, data transfer, and analysis.This project is supported by the Division of Advanced Cyberinfrastructure in the Directorate for Computer & Information Science & Engineering and the Physics Division in the Directorate of Mathematical and Physical Sciences.
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DOI: 10.1088/2632-2153/abab5f
发表时间: 2020-05
期刊: Machine Learning: Science and Technology
影响因子: --
作者: [R. Essick;P. Godwin;C. Hanna;L. Blackburn;E. Katsavounidis]
通讯作者: R. Essick;P. Godwin;C. Hanna;L. Blackburn;E. Katsavounidis
Discovering Neutron Stars and Black Holes with LIGO
CC* Compute: An Open Science Grid shared computing platform at Penn State
Framework: An A+ Framework for Multimessenger Astrophysics Discoveries through Real-Time Gravitational Wave Detection
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海外基金
化脓性链球菌分泌性酯酶Sse抑制LC3相关吞噬促其侵袭的机制研究
  • 批准号:
    --
  • 项目类别:
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  • 资助金额:
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  • 批准年份:
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  • 依托单位:
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  • 资助金额:
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  • 批准年份:
    2020
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  • 批准号:
    60776808
  • 项目类别:
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  • 资助金额:
    19.0万元
  • 批准年份:
    2007
  • 负责人:
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