Submillimeter Detectability of Gravitational-Wave Counterparts from Neutron-Star Mergers with the Xue-shan-mu-chang 15-meter Telescope

arXiv:2608.00770 · astro-ph.HE · Submitted 2026-08-01 · Read on arXiv

Di Xiao

astro-ph.HE

Submitted: 2026-08-01

Comments: 24 pages, 6 figures, accepted by ApJ

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

Terminology

• Consistency — 4× in this paper · explained in 3 episodes
• Core — 4× in this paper · explained in 2 episodes
• Aperture — 2× in this paper · explained in 1 episode
• Unified Framework — 2× in this paper · explained in 5 episodes
• AGN — 1× in this paper · explained in 1 episode
• Equal-Arrival-Time Surfaces — 1× in this paper

Sources

• Modeling Supernova-like Explosions Associated with Gamma-ray Bursts with Short Durations
• Probing Binary Neutron Star Merger Ejecta and Remnants with Gravitational Wave and Radio Observations
• The Deep Newtonian Regime in Late-Time Blast Waves: Inevitable Transition and Distinct Flux Signatures
• Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts
• GWTC-4.0: Population Properties of Merging Compact Binaries
• Scientific Objectives of the Xue-shan-mu-chang 15-meter Submillimeter Telescope

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