activity
20062023
most citedCompact radio emission indicates a structured jet was produced by a binary neutron star merger

395 citations · 1.5k across the 43 of their papers we have counts for

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20 papers · 1 filter

astro-ph.HE2023★ 6 cited

The spin measurement of MAXI J1348-630 using the Insight-HXMT data

Yujia Song, Nan Jia, Jun Yang +3

We report the results of fitting Insight-HXMT data to the black hole X-ray binary MAXI J1348-430, which was discovered on January 26th, 2019, with the Gas Slit Camera (GSC) on-boar…

astro-ph.HE2023★ 5 cited

The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3

Jun Yang, Federico García, Santiago del Palacio +6

Cygnus X-3 is a high-mass X-ray binary with a compact object accreting matter from a Wolf-Rayet donor star. Recently, it has been revealed by the Imaging X-ray Polarimetry Explorer…

astro-ph.HE2023★ 11 cited

One Fits All: A Unified Synchrotron Model Explains GRBs with FRED-Shaped Pulses

Zhen-Yu Yan, Jun Yang, Xiao-Hong Zhao +2

The analysis of gamma-ray burst (GRB) spectra often relies on empirical models lacking a distinct physical explanation. Previous attempts to couple physical models with observed da…

astro-ph.HE2023★ 11 cited

Multiwavelength Characterization of the High Mass X-ray Binary Population of M33

Margaret Lazzarini, Kyros Hinton, Cheyanne Shariat +12

We present multi-wavelength characterization of 65 high mass X-ray binary (HMXB) candidates in M33. We use the Chandra ACIS survey of M33 (ChASeM33) catalog to select hard X-ray po…

astro-ph.HE2023

Intermediate-Mass Black Holes: The Essential Population to Explore the Unified Model for Accretion and Ejection Processes

Xiaolong Yang, Jun Yang

We study radio and X-ray emissions from IMBHs and explore the unified model for accretion and ejection processes. The radio band survey of IMBH (candidate) hosted galaxies indicate…

astro-ph.HE2023★ 1 cited

Unveiling the small-scale jets in the rapidly growing supermassive black hole IZw1

Xiaolong Yang, Su Yao, Luigi C. Gallo +10

Accretion of black holes at near-Eddington or super-Eddington rates is the most powerful episode that drives black hole growth, and it may work in several types of objects. However…