Can we constrain the binary neutron star merger time from kilonova light curves?

arXiv:2610.28775 · astro-ph.HE, astro-ph.CO, gr-qc · Submitted 2026-10-20 · Read on arXiv

astro-ph.HE, astro-ph.CO, gr-qc

Submitted: 2026-10-20

Updated: 2026-10-20

Comments: 16 pages, 10 figures, 5 tables, submitted to A&A

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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