collaborators

6 papers

astro-ph.GA2026

\HI 21-cm Line Properties of the Nearby LIRG IRAS 04296+2923

Guixiang Feng, Zhongzu Wu, Chuanpeng Zhang +1

We present an analysis of archival Very Large Array (VLA) and Five-hundred-meter Aperture Spherical radio Telescope (FAST) \HI\ 21 cm data, together with archival multi-band radio…

astro-ph.HE2026

The FAST Discovery of a binary millisecond pulsar PSR~J1647-0156B (M12B) with a candidate cross matching algorithm

Qiuyu Yu, Yujie Wang, Zhichen Pan +9

We propose a pulsar candidate cross matching algorithm to sift radio pulsar search candidates from repeated observations of the same sky location such as globular clusters, high en…

astro-ph.GA2026

A jet-gas interaction beyond the host galaxy: detection of a neutral hydrogen outflow at cosmic noon

Renzhi Su, Stephen J. Curran, James R. Allison +6

We present upgraded Giant Metrewave Radio Telescope (uGMRT) observations of 0731+438, an \mbox{FR II} radio galaxy at a redshift of 2.429 with two lobes separated by 82 kpc. A blue…

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

Radio continuum and \HI 21-cm line observations of a nearby luminous infrared galaxy IRAS 17526+3253

Jianfeng Wu, Zhongzu Wu, Yulia Sotnikova +4

We present results from our EVN and GMRT observations of the radio continuum and spectral line emission in IRAS 17526+3253, along with an analysis of its arcsecond-scale radio prop…

astro-ph.HE2025

Discovery of a years-delayed radio flare from an unusually slow-evolved tidal disruption event

Zhumao Zhang, Xinwen Shu, Lei Yang +19

SDSS J1115+0544 is a unique low-ionization nuclear emission-line region (LINER) galaxy with energetic ultraviolet (UV), optical and mid-infrared outbursts occurring in its nucleus.…