Cyberinfrastructure Requirements to Enhance Multi-messenger Astrophysics. Chang, P., Allen, G., Anderson, W., Bianco, F., B., Bloom, J., S., Brady, P., R., Brazier, A., Cenko, S., B., Couch, S., M., DeYoung, T., Deelman, E., Etienne, Z., B., Foley, R., J., Fox, D., B., Golkhou, V., Z., Grant, D., R., Hanna, C., Holley-Bockelmann, K., Howell, D., A., Huerta, E., A., Johnson, M., W., G., Juric, M., Kaplan, D., L., Katz, D., S., Keivani, A., Kerzendorf, W., Kopper, C., Lam, M., T., Lehner, L., Marka, Z., Marka, S., Nabrzyski, J., Narayan, G., O'Shea, B., W., Petravick, D., Quick, R., Street, R., A., Taboada, I., Timmes, F., Turk, M., J., Weltman, A., & Zhang, Z. 3, 2019. Paper Website abstract bibtex 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.
@article{
title = {Cyberinfrastructure Requirements to Enhance Multi-messenger Astrophysics},
type = {article},
year = {2019},
websites = {http://arxiv.org/abs/1903.04590},
month = {3},
day = {11},
id = {2bcb05ba-9331-34ad-b009-f2f4cba04f58},
created = {2020-04-22T21:44:57.173Z},
accessed = {2020-04-22},
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profile_id = {42d295c0-0737-38d6-8b43-508cab6ea85d},
last_modified = {2020-05-11T14:43:33.833Z},
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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.},
bibtype = {article},
author = {Chang, Philip and Allen, Gabrielle and Anderson, Warren and Bianco, Federica B. and Bloom, Joshua S. and Brady, Patrick R. and Brazier, Adam and Cenko, S. Bradley and Couch, Sean M. and DeYoung, Tyce and Deelman, Ewa and Etienne, Zachariah B and Foley, Ryan J. and Fox, Derek B and Golkhou, V. Zach and Grant, Darren R and Hanna, Chad and Holley-Bockelmann, Kelly and Howell, D. Andrew and Huerta, E. A. and Johnson, Margaret W. G. and Juric, Mario and Kaplan, David L. and Katz, Daniel S. and Keivani, Azadeh and Kerzendorf, Wolfgang and Kopper, Claudio and Lam, Michael T. and Lehner, Luis and Marka, Zsuzsa and Marka, Szabolcs and Nabrzyski, Jarek and Narayan, Gautham and O'Shea, Brian W. and Petravick, Donald and Quick, Rob and Street, Rachel A. and Taboada, Ignacio and Timmes, Frank and Turk, Matthew J. and Weltman, Amanda and Zhang, Zhao}
}
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