Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories

Context. 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, such as the V...

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Bibliographic Details

Main Authors:	Loffredo, Eleonora (Author) , Hazra, N. (Author) , Dupletsa, U. (Author) , Branchesi, M. (Author) , Ronchini, S. (Author) , Santoliquido, F. (Author) , Perego, A. (Author) , Banerjee, B. (Author) , Bisero, S. (Author) , Ricigliano, G. (Author) , Vergani, S. (Author) , Andreoni, I. (Author) , Cantiello, M. (Author) , Harms, J. (Author) , Mapelli, Michela (Author) , Oganesyan, G. (Author)
Format:	Article (Journal)
Language:	English
Published:	06 May 2025
In:	Astronomy and astrophysics Year: 2025, Volume: 697, Pages: 1-35
ISSN:	1432-0746
DOI:	10.1051/0004-6361/202452863
Online Access:	Verlag, kostenfrei, Volltext: https://doi.org/10.1051/0004-6361/202452863 Verlag, kostenfrei, Volltext: https://www.aanda.org/10.1051/0004-6361/202452863
Author Notes:	E. Loffredo, N. Hazra, U. Dupletsa, M. Branchesi, S. Ronchini, F. Santoliquido, A. Perego, B. Banerjee, S. Bisero, G. Ricigliano, S. Vergani, I. Andreoni, M. Cantiello, J. Harms, M. Mapelli, and G. Oganesyan