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From the 2 of 5 linked papers with an AI index.

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5 papers

astro-ph.HE2026

Radio and X-ray flux rebrightening six years after outburst in a partially-obscured extreme changing-look AGN

Tianyao Zhou, Xinwen Shu, Lei Yang +14

The paper reports multi‑year observations of the partially obscured AGN SDSS J1548+2208, revealing sustained high mid‑infrared and hard X‑ray fluxes and a late‑time radio rebrighte…

astro-ph.HE2026

AT2019ijn: a fast-rising, slow-decaying blue optical transient with exceptionally bright radio emission

Hucheng Ding, Xinwen Shu, Luming Sun +9

We report the discovery of a peculiar optical transient, AT2019ijn, occurred in the nuclear region of a dwarf galaxy at z=0.273. It rises rapidly to peak at a luminosity of Mg=-21.…

astro-ph.HE2026

Dust-obscured radio-emitting tidal disruption event coincident with a high-energy neutrino event

Tianyao Zhou, Xinwen Shu, Guobin Mou +14

Despite the growing number of high-energy neutrinos (TeV-PeV) detected by IceCube, their astrophysical origins remain largely unidentified. Recent observations have linked a few ti…

astro-ph.GA2025

The distance of quasar outflows from the central source: The first consistent values from emission and absorption determinations

Mayank Sharma, Nahum Arav, Qinyuan Zhao +8

Measuring the distance of quasar outflows from the central source () is essential for determining their importance for AGN feedback. There are two methods to measure : 1) A d…

astro-ph.GA2025

Galactic-scale emission-line outflow from the radio-loud quasar 3C 191

Qinyuan Zhao, Luming Sun, Lu Shen +6

Quasar feedback is routinely invoked as an indispensable ingredient in galaxy formation models. Galactic outflows are a crucial agent of quasar feedback that frequently manifest th…