Gravity Spy: lessons learned and a path forward

被引:0
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作者
Michael Zevin
Corey B. Jackson
Zoheyr Doctor
Yunan Wu
Carsten Østerlund
L. Clifton Johnson
Christopher P. L. Berry
Kevin Crowston
Scott B. Coughlin
Vicky Kalogera
Sharan Banagiri
Derek Davis
Jane Glanzer
Renzhi Hao
Aggelos K. Katsaggelos
Oli Patane
Jennifer Sanchez
Joshua Smith
Siddharth Soni
Laura Trouille
Marissa Walker
Irina Aerith
Wilfried Domainko
Victor-Georges Baranowski
Gerhard Niklasch
Barbara Téglás
机构
[1] The University of Chicago,Kavli Institute for Cosmological Physics
[2] The University of Chicago,Enrico Fermi Institute
[3] University of Wisconsin–Madison,Information School
[4] Northwestern University,Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA)
[5] Northwestern University,Department of Electrical and Computer Engineering
[6] Syracuse University,School of Information Studies
[7] The Adler Planetarium,Zooniverse
[8] University of Glasgow,SUPA, School of Physics and Astronomy
[9] Northwestern University,Department of Physics and Astronomy
[10] California Institute of Technology,LIGO Laboratory
[11] Louisiana State University,Department of Physics and Astronomy
[12] LIGO Hanford Observatory,The Nicholas and Lee Begovich Center for Gravitational
[13] California State University Fullerton,Wave Physics and Astronomy
[14] Massachusetts Institute of Technology,LIGO Laboratory
[15] Christopher Newport University,Department of Physics, Computer Science and Engineering
[16] Sorbonne Paris Nord University,undefined
[17] ConSol Software GmbH,undefined
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摘要
The Gravity Spy project aims to uncover the origins of glitches, transient bursts of noise that hamper analysis of gravitational-wave data. By using both the work of citizen-science volunteers and machine learning algorithms, the Gravity Spy project enables reliable classification of glitches. Citizen science and machine learning are intrinsically coupled within the Gravity Spy framework, with machine learning classifications providing a rapid first-pass classification of the dataset and enabling tiered volunteer training, and volunteer-based classifications verifying the machine classifications, bolstering the machine learning training set and identifying new morphological classes of glitches. These classifications are now routinely used in studies characterizing the performance of the LIGO gravitational-wave detectors. Providing the volunteers with a training framework that teaches them to classify a wide range of glitches, as well as additional tools to aid their investigations of interesting glitches, empowers them to make discoveries of new classes of glitches. This demonstrates that, when giving suitable support, volunteers can go beyond simple classification tasks to identify new features in data at a level comparable to domain experts. The Gravity Spy project is now providing volunteers with more complicated data that includes auxiliary monitors of the detector to identify the root cause of glitches.
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