activity
20232025
most citedNICER, NuSTAR and Insight-HXMT views to the newly discovered black hole X-ray binary Swift J1727.8--1613

45 citations · 90 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2025★ 1 cited

The peculiar disk evolution of 4U 1630--472 observed by Insight-HXMT during the 2022 and 2023 outbursts

Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui +10

We study the spectral properties of the black hole X-ray transient binary 4U 1630--472 during the 2022 and 2023 outbursts with Insight-HXMT observations. We find that the outbursts…

astro-ph.HE2025★ 7 cited

Insight-HXMT, NICER and NuSTAR views to the newly discovered black hole X-ray binary Swift J151857.0--572147

Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui +10

The systematic properties are largely unknown for the black hole X-ray binary Swift J151857.0--572147 newly discovered in the 2024 outburst. The nature of a black hole can be compl…

astro-ph.HE2025★ 9 cited

NICER, NuSTAR and Insight-HXMT views to black hole X-ray binary SLX 1746--331

Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui +13

We study the spectral and temporal properties of the black hole X-ray transient binary SLX 1746--331 during the 2023 outburst with NICER, NuSTAR, and Insight-HXMT observations. Thr…

astro-ph.HE2025★ 45 cited

NICER, NuSTAR and Insight-HXMT views to the newly discovered black hole X-ray binary Swift J1727.8--1613

Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui +13

Swift J1727.8--1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER and NuSTAR observations when the sourc…

astro-ph.HE2025★ 9 cited

Back to business: SLX 1746--331 after 13 years of silence

Jing-Qiang Peng, Shu Zhang, Peng-Ju Wang +17

The black hole candidate system SLX 1746--331 was back to business in 2023, after a long silence of roughly 13 years. An outburst was observed thoroughly by \textit{Insight}-HXMT a…

astro-ph.HE2024

A Phase-resolved View of "Heartbeat"-like variability in IGR J17091-3624 During the 2022 Outburst

Qing-Cang Shui, Shu Zhang, Jing-Qiang Peng +9

IGR J17091-3624, in addition to GRS 1915+105, is the only black hole X-ray binary that displays ``heartbeat"-like variability characterized by structured flares with high amplitude…

astro-ph.HE2024

Phase-resolved Spectroscopy of Low-frequency Quasi-periodic Oscillations from the Newly Discovered Black Hole X-ray Binary Swift J1727.8-1613

Qing-Cang Shui, Shu Zhang, Jiang-Qiang Peng +14

Low-frequency quasi-periodic oscillations (LFQPOs) are commonly observed in X-ray light curves of black hole X-ray binaries (BHXRBs); however, their origin remains a topic of debat…

astro-ph.HE2024

Recovery of High-energy Low-frequency Quasi-periodic Oscillations from Black Hole X-ray Binary MAXI J1535-571 with a Hilbert-Huang Transform Method

Qingcang Shui, Shu Zhang, Shuangnan Zhang +15

We propose a method based on the Hilbert-Huang transform (HHT) to recover the high-energy waveform of low-frequency quasi-periodic oscillations (LFQPOs). Based on the method, we su…

astro-ph.HE2023★ 19 cited

A Phase-resolved View of the Low-frequency Quasiperiodic Oscillations from the Black Hole Binary MAXI J1820+070

Qing C. Shui, S. Zhang, Shuang N. Zhang +21

Although low-frequency quasiperiodic oscillations (LFQPOs) are commonly detected in the X-ray light curves of accreting black hole X-ray binaries, their origin still remains elusiv…