Prospects for optical detections from binary neutron star mergers with the next-generation multi-mes...
Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
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Author / Creator
Loffredo, E , Hazra, N , Dupletsa, U , Branchesi, M , Ronchini, S , Santoliquido, F , Perego, A , Banerjee, B , Bisero, S , Ricigliano, G , Vergani, S , Andreoni, I , Cantiello, M , Harms, J , Mapelli, M and Oganesyan, G
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Next-generation gravitational wave (GW) observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, will observe binary neutron star (BNS) mergers across cosmic history, providing precise parameter estimates for the closest ones. Innovative wide-field observatories, like the Vera Rubin Observatory, will quickly cover large portions of t...
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Full title
Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
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TN_cdi_proquest_journals_3124189694
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3124189694
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E-ISSN
2331-8422
