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20242026
most citedX-ray spectropolarimetric characterization of the Z-source GX 340+0 in the normal branch

4 citations · 5 across the 13 of their papers we have counts for

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astro-ph.HE2026

X-rays breaking out of pre-explosion ejecta mark a supernova's first light

Weimin Yuan, Qiu-Ju Huang, Jin-Ping Zhu +130

Massive stars die as core-collapse supernovae, whose optical light emerges days after the implosion. Theory predicts that the initial collapse-driven shock, upon breaking through t…

astro-ph.HE2026

Discovery of EP J175257.3-351923 as a Candidate Black Hole Low-Mass X-ray Binary

G. L. Huang, Q. C. Zhao, L. Tao +30

We report the discovery of a new X-ray transient, EP J175257.3-351923 (EP250916a), by the Einstein Probe (EP) near the Galactic plane. The outburst lasted for at least 250\,days, r…

astro-ph.HE2026

Unveiling hidden millihertz quasi-periodic oscillations in 1A 0535+262

Zihan Yang, Ruican Ma, Mariano Méndez +9

Be/X-ray binary pulsars show transient outbursts and complex timing behaviour, including millihertz quasi-periodic oscillations (QPOs), whose physical origin and energy dependence…

astro-ph.HE2026

Deep VLBI constraints on compact radio cores in four ultraluminous X-ray sources

Ailing Wang, Hua Feng, Tao An +7

We present high-sensitivity Very Long Baseline Interferometry (VLBI) observations of four ultraluminous X-ray sources (ULXs): Holmberg II X-1, IC 342 X-1, NGC 6946 X-1, and NGC 925…

astro-ph.HE2026

Discovery of energy-dependent phase variations in the polarization angle of Cen X-3

Qing-Chang Zhao, Lian Tao, Sergey S. Tsygankov +7

We present a detailed polarimetric analysis of Cen X-3 using \ixpe observations during its high state, revealing complex energy-dependent polarization behavior. While phase-average…

astro-ph.HE2025

The First X-ray Polarimetry of GRS 1739--278 Reveals Its Rapidly Spinning Black Hole

Qing-Chang Zhao, Michal Dovciak, Han-Cheng Li +6

We present a joint spectro-polarimetric analysis of the black hole X-ray binary GRS~1739--278 during its 2025 mini-outburst, using simultaneous observations from \ixpe\ and \nustar…

astro-ph.HE2025★ 1 cited

A fast powerful X-ray transient from possible tidal disruption of a white dwarf

Dongyue Li, Wenda Zhang, Jun Yang +97

Stars captured by black holes (BHs) can be torn apart by strong tidal forces, producing electromagnetic flares. To date, more than 100 tidal disruption events (TDEs) have been obse…

astro-ph.HE2025

Multiwavelength Observations of the Apparently Non-repeating FRB 20250316A

Ye Li, Hui Sun, Lei Qian +72

The physical origin of fast radio bursts (FRBs) remains uncertain. Although multiwavelength observations have been widely conducted, only Galactic FRB~20200428D is associated with…

astro-ph.HE2025★ 4 cited

X-ray spectropolarimetric characterization of the Z-source GX 340+0 in the normal branch

Fabio La Monaca, Alessandro Di Marco, Francesco Coti Zelati +11

This study presents an X-ray spectropolarimetric characterisation of the Z-source GX 340+0 during the normal branch (NB) and compares it with that obtained for the horizontal branc…

astro-ph.HE2025

X-ray Polarimetry in the Low Statistics Regime using the Bayesian Approach Reveals Polarization Angle Variations

Hong Li, Qing-Chang Zhao, Hua Feng +2

X-ray polarimetry of accreting compact objects has revealed fast time variations in the polarization angle (PA), suggesting that the geometry and/or optical depth of the Comptoniza…

astro-ph.HE2024

Continuous evolution of the polarization properties in the transient X-ray pulsar RX J0440.9+4431/LS V +44 17

Q. C. Zhao, L. Tao, S. Sergey Tsygankov +6

We present a detailed time-resolved and phase-resolved polarimetric analysis of the transient X-ray pulsar RX J0440.9+4431/LS V +44 17, using data from the Imaging X-ray Polarimetr…

astro-ph.HE2024

Discovery of Rapid Polarization Angle Variation During the 2022 Outburst of XTE J1701-462

QingChang Zhao, Hong Li, Lian Tao +1

The geometry of the Comptonization corona in neutron star low-mass X-ray binaries is still unclear. We conducted time-resolved polarimetric analysis of the archival observations of…

astro-ph.HE2024

Magnetic accretion flow explains the hysteresis q-diagram seen in outbursts of black hole low-mass X-ray binaries

Jiahui Huang, Hua Feng, Lian Tao

Black hole low-mass X-ray binaries undergo quiescence-outburst cycles. During the outbursts, they typically go through a q-shaped pattern in the hardness-intensity diagram (HID), k…