CA17137 - 5th MC virtual meeting

Europe/Rome
Topic: g2net CA17137 meeting Time: Sep 2, 2021 02:00 PM Rome Join Zoom Meeting https://us02web.zoom.us/j/88189972733?pwd=VXN6MVhYNFFtZ09UeXkyMTBpYlBzdz09 Meeting ID: 881 8997 2733 Passcode: 070763 One tap mobile +3902124128823,,88189972733#,,,,*070763# Italy +390694806488,,88189972733#,,,,*070763# Italy Dial by your location +39 021 241 28 823 Italy +39 069 480 6488 Italy +39 020 066 7245 Italy +1 301 715 8592 US (Washington DC) +1 312 626 6799 US (Chicago) +1 346 248 7799 US (Houston) +1 646 558 8656 US (New York) +1 669 900 9128 US (San Jose) +1 253 215 8782 US (Tacoma) Meeting ID: 881 8997 2733 Passcode: 070763 Find your local number: https://us02web.zoom.us/u/kvZoXI2ER
Elena Cuoco
Description

The breakthrough discovery of gravitational waves on September 14, 2015 was made possible through synergy of techniques drawing from expertise in physics, mathematics, information science and computing.  At present, there is a rapidly growing interest in Machine Learning (ML), Deep Learning (DL), classification problems, data mining and visualization and, in general, in the development of new techniques and algorithms for efficiently handling the complex and massive data sets found in what has been coined "Big Data", across a broad range of disciplines, ranging from Social Sciences to Natural Sciences. The rapid increase in computing power at our disposal and the development of innovative techniques for the rapid analysis of data will be vital to the exciting new field of Gravitational Wave (GW) Astronomy, on specific topics such as control and feedback systems for next-generation detectors, noise removal, data analysis and data-conditioning tools.The discovery of GW signals from colliding binary black holes (BBH) and the likely existence of a newly observable population of massive, stellar-origin black holes, has made the analysis of low-frequency GW data a crucial mission of GW science. The low-frequency performance of Earth-based GW detectors is largely influenced by the capability of handling ambient seismic noise suppression. This Cost Action aims at creating a broad network of scientists from four different areas of expertise, namely GW physics, Geophysics, Computing Science and Robotics, with a common goal of tackling challenges in data analysis and noise characterization for GW detectors.

G2net website: https://www.g2net.eu

This the 5th g2net MC meeting and the 2nd g2net MC virtual meeting

 

Registration
Participants
    • 9:00 AM 9:15 AM
      Welcome to participants

      1) Welcome to participants
      2) Verification of the presence of two-thirds of the
      Participating COST Countries
      3) Adoption of agenda

      Convener: Elena Cuoco
    • 9:15 AM 9:55 AM
      Update by the Action Chair
      Convener: Elena Cuoco
    • 9:55 AM 10:05 AM
      Update from the COST Association
    • 10:05 AM 11:55 AM
      Follow-up of MoU objectives: progress report of working groups
      • 10:05 AM
        Updates by WG1 leader 10m
      • 10:15 AM
        Updates by WG2 leader 10m
      • 10:25 AM
        Updates by WG3 leader 10m
      • 10:35 AM
        Updates by SCM coordinator 10m
      • 10:45 AM
        Updates by STSM coordinator 10m
      • 10:55 AM
        Coffee break 20m
      • 11:15 AM
        Updates by DA coordinator 10m
      • 11:25 AM
        Updates on dissemination 10m
      • 11:35 AM
        Updates by Stakeholder coordinator 10m
      • 11:45 AM
        Report on Kaggle competition, status and plan 10m
    • 11:55 AM 12:15 PM
      Annotated rules from 1 November 2021
    • 12:15 PM 12:30 PM
      Scientific planning

      a) Scientific strategy (MoU objectives, GP Goals, WG
      tasks and deliverables).
      b) Action Budget Planning (Define which are the objectives,
      milestones, deliverables in the next year and
      WBP4)

    • 12:30 PM 12:50 PM
      Organization/dicussion/vote
    • 12:50 PM 1:00 PM
      Summary of MC decisions, closing