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20022026
most citedAn Explanation for the soft X-ray excess in AGN

479 citations · 4.2k across the 85 of their papers we have counts for

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10 papers · 1 filter

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★ 62 cited

A Systematic View of Ten New Black Hole Spins

Paul A. Draghis, Jon M. Miller, Abderahmen Zoghbi +4

The launch of NuSTAR and the increasing number of binary black hole (BBH) mergers detected through gravitational wave (GW) observations have exponentially advanced our understandin…

astro-ph.HE2022★ 11 cited

The multi-epoch X-ray tale of I Zwicky 1 outflows

Daniele Rogantini, Elisa Costantini, Luigi Gallo +3

The narrow-line Seyfert 1 galaxy I Zwicky 1 shows a unique and complex system of ionised gas in outflow, which consists of an ultra-fast wind and a two-component warm absorber. In…

astro-ph.HE2022★ 3 cited

Comparing Reflection and Absorption Models for the Soft X-ray Variability in the NLS1 AGN UGC 11763

Jiachen Jiang, Luigi C. Gallo, Dirk Grupe +1

We present a spectral analysis of two XMM-Newton observations of the narrow-line Seyfert 1 galaxy UGC 11763. UGC 11763 shows very different soft X-ray spectral shapes in the two ob…

astro-ph.HE2022★ 4 cited

The Low Temperature Corona in ESO 511G030 Revealed by NuSTAR and XMM-Newton

Zuobin Zhang, Jiachen Jiang, Honghui Liu +9

We present the results from a coordinated XMM-Newton NuSTAR observation of the Seyfert 1 Galaxy ESO 511G030. With this joint monitoring programme, we conduct a detailed vari…

astro-ph.HE2022★ 1 cited

A truncated inner disc in the Seyfert 1 galaxy WKK 4438

L. C. Gallo, M. Z. Buhariwalla, J. Jiang +2

Understanding if and when the accretion disc extends down to the innermost stable circular orbit (ISCO) is important since it is the fundamental assumption behind measuring black h…