arXiv · 1903.04590
Cyberinfrastructure Requirements to Enhance Multi-messenger Astrophysics
Abstract
The identification of the electromagnetic counterpart of the gravitational wave event, GW170817, and discovery of neutrinos and gamma-rays from TXS 0506+056 heralded the new era of multi-messenger astrophysics. As the number of multi-messenger events rapidly grow over the next decade, the cyberinfrastructure requirements to handle the increase in data rates, data volume, need for event follow up, and analysis across the different messengers will also explosively grow. The cyberinfrastructure requirements to enhance multi-messenger astrophysics will both be a major challenge and opportunity for astronomers, physicists, computer scientists and cyberinfrastructure specialists. Here we outline some of these requirements and argue for a distributed cyberinfrastructure institute for multi-messenger astrophysics to meet these challenges.
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Philip Chang, Gabrielle Allen, Warren Anderson, Federica B. Bianco, Joshua S. Bloom, Patrick R. Brady, Adam Brazier, S. Bradley Cenko, Sean M. Couch, Tyce DeYoung, Ewa Deelman, Zachariah B Etienne, Ryan J. Foley, Derek B Fox, V. Zach Golkhou, Darren R Grant, Chad Hanna, Kelly Holley-Bockelmann, D. Andrew Howell, E. A. Huerta, Margaret W. G. Johnson, Mario Juric, David L. Kaplan, Daniel S. Katz, Azadeh Keivani, Wolfgang Kerzendorf, Claudio Kopper, Michael T. Lam, Luis Lehner, Zsuzsa Marka, Szabolcs Marka, Jarek Nabrzyski, Gautham Narayan, Brian W. O'Shea, Donald Petravick, Rob Quick, Rachel A. Street, Ignacio Taboada, Frank Timmes, Matthew J. Turk, Amanda Weltman, Zhao Zhang. 2019-03-11. Cyberinfrastructure Requirements to Enhance Multi-messenger Astrophysics. https://arxiv.org/abs/1903.04590
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