activity
20102022
most citedPossible ~0.4 hour X-ray quasi-periodicity from an ultrasoft active galactic nucleus

25 citations · 57 across the 5 of their papers we have counts for

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astro-ph.HE2022

Response of the Fe K_alpha line emission to the X-ray continuum variability in the changing-look active galactic nucleus NGC 1566

W. C. Liang, X. W. Shu, J. X. Wang +5

NGC 1566 is a changing look AGN known to exhibit recurrent X-ray outbursts with each lasting for several years. The most recent X-ray outburst is observed on 2018, with a substanti…

astro-ph.HE2022★ 19 cited

Discovery of late-time X-ray flare and anomalous emission line enhancement after the nuclear optical outburst in a narrow-line Seyfert 1 Galaxy

W. J. Zhang, X. W. Shu, Z. F. Sheng +7

CSS J102913+404220 is a peculiar narrow line Seyfert 1 galaxy with an energetic nuclear optical outburst. We present a detailed analysis of its multi-wavelength photometric and spe…

astro-ph.HE2021

Completing the X-ray view of the recently discovered supernova remnant G53.41+0.03

V. Domček, J. Vink, P. Zhou +2

Aims: We present a detailed X-ray study of the recently discovered supernova remnant (SNR) G53.41+0.03 that follows up and further expands on the previous, limited analysis of arch…

astro-ph.HE2020★ 25 cited

Possible ~0.4 hour X-ray quasi-periodicity from an ultrasoft active galactic nucleus

J. R. Song, X. W. Shu, L. M. Sun +6

RX J1301.9+2747 is an ultrasoft active galactic nucleus (AGN) with unusual X-ray variability that is characterized by a long quiescent state and a short-lived flare state. The X-ra…

astro-ph.HE2010★ 13 cited

On the Relation of Hard X-ray Peak Flux and Outburst Waiting Time in the Black Hole Transient GX 339-4

Y. X. Wu, W. Yu, Z. Yan +2

Aims. In this work we re-investigated the empirical relation between the hard X-ray peak flux and the outburst waiting time found previously in the black hole transient GX 339-4. W…