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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33 papers · 1 filter

astro-ph.HE2025★ 6 cited

Prospects for Time-Domain and Multi-Messenger Science with eXTP

Shu-Xu Yi, Wen Zhao, Ren-Xin Xu +75

In this new era of time-domain and multi-messenger astronomy, various new transients and new phenomena are constantly being discovered thanks to the rapid advances in observations,…

astro-ph.HE2023★ 13 cited

Dimming of Continuum Captured in Mrk 841: New Clues on the Nature of the Soft X-ray Excess

Missagh Mehdipour, Gerard Kriss, Jelle Kaastra +2

We report on a remarkable change in the spectral energy distribution (SED) of Mrk 841, providing new insights on how the soft X-ray excess emission in active galactic nuclei (AGNs)…

astro-ph.HE2023

XMM-Newton Reflection Grating Spectrometer

Junjie Mao, Frits Paerels, Matteo Guainazzi +1

The past two decades have witnessed the rapid growth of our knowledge of the X-ray Universe thanks to flagship X-ray space observatories like XMM-Newton and Chandra. A significant…

astro-ph.HE2023★ 8 cited

The Collisional and Photoionized Plasma in the Polarized NLS1 galaxy Mrk 1239

Margaret Z. Buhariwalla, Luigi C. Gallo, J. Mao +4

Mrk 1239 is a highly polarized NLS1 in the optical band, whose keV spectrum has remained remarkably consistent over more than two decades of observation. Previous analysis…

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.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…