activity
20202026
most citedTiming properties of the X-ray accreting pulsar 1A 0535+262 studied with Insight-HXMT

22 citations · 114 across the 18 of their papers we have counts for

collaborators

16 papers

astro-ph.HE2026★ 1 cited

IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

Jack T. Dinsmore, Roger W. Romani, S. Zhang +9

The Lighthouse pulsar (PSR J11016101) sports a bright X-ray trail and filament. The synchrotron emission from both structures is expected to be polarized, with electric vector p…

astro-ph.HE2025★ 4 cited

Insight-HXMT observations on thermonuclear X-ray bursts from 4U~1608--52 in the low/hard state: the energy-dependant hard X-ray deficit and cooling saturation of the corona

Y. P. Chen, S. Zhang, L. Ji +9

During thermonuclear bursts, it is suspected that {\bf the cooling of the corona by the burst emission} may be the cause of hard X-ray {\bf deficits}. Although this {\bf deficit} h…

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

estimating the spin of MAXI J1348--630 from intermediate and soft states using \textit{Insight}-HXMT data

J. Guan, R. C. Ma, L. Tao +6

We present a broadband spectral analysis of the soft-intermediate and soft states using \textit{Insight}-HXMT observations of the black hole binary MAXI J1348--630 during its outbu…

astro-ph.HE2024

A Revised Spin of the Black Hole in GRS 1716-249 with a New Distance

S. J. Zhao, L. Tao, Q. Q. Yin +12

GRS 1716-249 is a stellar-mass black hole in a low-mass X-ray binary that underwent a gaint outburst in 2016/17. In this paper we use simultaneous observations of Insight-HXMT and…

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…

astro-ph.HE2022★ 12 cited

Trace the Accretion Geometry of H 1743--322 with Type C Quasi-periodic Oscillations in Multiple Outbursts

Qing-Cang Shui, Shu Zhang, Yu-Peng P. Chen +12

We present a systematic analysis of type C quasi-periodic oscillation (QPO) observations of H 1743--322 throughout the Rossi X-ray Timing Explorer (RXTE) era. We find that, while d…

astro-ph.HE2022★ 1 cited

Monte-Carlo simulations on possible collimation effects of outflows to fan-beamed emission of ultraluminous accreting X-ray pulsars

X. Hou, Y. You, L. Ji +10

Pulsating ultraluminous X-ray sources (PULXs) are accreting pulsars with apparent X-ray luminosity exceeding . We perform Monte-Carlo simulations to inve…

astro-ph.HE2022★ 1 cited

Fan beamed X-ray emission from 1 keV to above 130 keV from the ultraluminous X-ray pulsar RX J0209.6-7427 in the Small Magellanic Cloud

X. Hou, M. Y. Ge, L. Ji +10

We present detailed timing and spectral analyses of the transient X-ray pulsar RX J0209.67427 in the Small Magellanic Cloud during its 2019 giant outburst. With a better known d…

astro-ph.HE2022★ 22 cited

Timing properties of the X-ray accreting pulsar 1A 0535+262 studied with Insight-HXMT

P. J. Wang, L. D. Kong, S. Zhang +13

We report results on the timing analysis of the 2020 giant outburst of 1A 0535+262, using broadband data from Insight-HXMT. The analysis of the pulse profile evolution from the sub…

astro-ph.HE2022★ 14 cited

The peculiar spectral evolution of the new X-ray transient MAXI J0637-430

R. C. Ma, R. Soria, L. Tao +15

We studied the transient Galactic black hole candidate MAXI J0637-430 with data from Insight-HXMT, Swift and XMM-Newton. The broad-band X-ray observations from Insight-HXMT help us…

astro-ph.HE2022★ 11 cited

Variations of cyclotron resonant scattering features in Vela X-1 revealed with Insight-HXMT

Q. Liu, W. Wang, X. Chen +6

We present a detailed study of the high mass X-ray binary Vela X-1, using observations performed by Insight-HXMT in 2019 and 2020, concentrating on timing analysis and spectral stu…

astro-ph.HE2022★ 9 cited

Evolution of Accretion Modes between Spectral States Inferred from Spectral and Timing Analysis of Cygnus X-1 with Insight-HXMT observations

M. Z. Feng, L. D. Kong, P. J. Wang +14

We execute a detailed spectral-timing study of Cygnus X-1 in the low/hard, intermediate and high/soft states with the Hard X-ray Modulation Telescope observations. The broad band e…

astro-ph.HE2021★ 5 cited

X-ray spectral-timing variability of 1A 0535+262 during the 2020 giant outburst

P. Reig, R. C. Ma, L. Tao +3

The Be/X-ray binary 1A 0535+262 underwent a giant X-ray outburst in November 2020, peaking at erg s (1--100 keV, 1.8 kpc), the brightest outburst recor…

astro-ph.HE2020★ 11 cited

The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition

L. J. Wang, M. Y. Ge, J. S. Wang +6

In Dec. 2011 PSR B0540-69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by ~36%. About 1000 days after the SRT, the X-ray l…