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From the 2 of 12 linked papers with an AI index.

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12 papers

astro-ph.IM2026

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope

Ulyana Dupletsa, Francesco Iacovelli, Mikhail Korobko +23

The paper evaluates how different design choices and noise characteristics of the Einstein Telescope affect its ability to detect and analyze various gravitational‑wave sources, us…

astro-ph.HE2026

The ultra-fast afterglow of GRB 260226A

Biswajit Banerjee, Alessio Mei, Annarita Ierardi +13

The paper presents Fermi LAT observations of GRB 260226A that captured an unprecedented number of >100 MeV photons, enabling a detailed reconstruction of the early afterglow which…

astro-ph.HE2026

Detectability of Gravitational-wave counterparts of EP-FXTs observed during the O4b LIGO-Virgo-KAGRA Observing Run

Ansh Chopra, Samuele Ronchini, Biswajit Banerjee +5

Fast X-ray transients (FXTs) detected by the Einstein Probe mission have emerged as a rapidly growing class of extragalactic transients, whose physical origin remains uncertain. Co…

astro-ph.HE2026

MeV absorption in gamma-ray bursts as a probe of their progenitor environments

Gor Oganesyan, Om Sharan Salafia, Emanuele Sobacchi +8

A small fraction of X-ray photons from -ray bursts (GRBs), after escaping the relativistic jet, are scattered by electrons in the circumburst medium. Subsequent photon-photon a…

astro-ph.HE2026

Gravitational wave detectability range informed by external messengers

S. Ronchini, A. Chopra, T. Dal Canton +3

A rapid estimate of gravitational-wave (GW) detectability associated with astronomical transients is crucial for optimizing multi-messenger follow-up strategies and for constrainin…

astro-ph.HE2025

Early X-ray emission of short Gamma-Ray Bursts: insights into physics and multi-messenger prospects

Annarita Ierardi, Gor Oganesyan, Stefano Ascenzi +3

Early X-ray emission of Gamma-Ray Bursts (GRBs) traces the transition between the prompt emission and the afterglow radiation, and its rapid flux decline is often interpreted as th…