activity
20092025
most citedRadial metal abundance profiles in the intra-cluster medium of cool-core galaxy clusters, groups, and ellipticals

121 citations · 1k across the 48 of their papers we have counts for

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Showing 2022Show all

8 papers · 1 filter

physics.atom-ph2022★ 6 cited

R-matrix electron-impact excitation data for the H- and He-like ions with Z=6-30

Junjie Mao, G. Del Zanna, Liyi Gu +2

Plasma models built on extensive atomic data are essential to interpreting the observed cosmic spectra. H-like Lyman series and He-like triplets observable in the X-ray band are po…

astro-ph.HE2022★ 17 cited

Multi-wavelength observations of the obscuring wind in the radio-quiet quasar MR 2251-178

Junjie Mao, G. A. Kriss, H. Landt +11

Obscuring winds driven away from active supermassive black holes are rarely seen due to their transient nature. They have been observed with multi-wavelength observations in a few…

astro-ph.SR2022★ 8 cited

Searching for cataclysmic variable stars in unidentified X-ray sources

J. Takata, X. F. Wang, A. K. H. Kong +6

We carry out a photometric search for new cataclysmic variable stars (CVs), with the goal of identification for candidates of AR~Scorpii-type binary systems. We select GAIA sources…

astro-ph.HE2022★ 18 cited

10-Year Transformation of the Obscuring Wind in NGC 5548

Missagh Mehdipour, Gerard A. Kriss, Elisa Costantini +4

A decade ago the archetypal Seyfert-1 galaxy NGC 5548 was discovered to have undergone major spectral changes. The soft X-ray flux had dropped by a factor of 30 while new broad and…

astro-ph.HE2022★ 5 cited

Detection of an Unidentified Soft X-ray Emission Feature in NGC 5548

Liyi Gu, Junjie Mao, Jelle S. Kaastra +17

NGC~5548 is an X-ray bright Seyfert 1 active galaxy. It exhibits a variety of spectroscopic features in the soft X-ray band, including in particular the absorption by the AGN outfl…

astro-ph.HE2022★ 14 cited

X-ray spectra of the Fe-L complex III: systematic uncertainties in the atomic data

Liyi Gu, Chintan Shah, Junjie Mao +14

There has been a growing request from the X-ray astronomy community for a quantitative estimate of systematic uncertainties originating from the atomic data used in plasma codes. T…