activity
20142024
most citedUsing iron line reverberation and spectroscopy to distinguish Kerr and non-Kerr black holes

64 citations · 171 across the 16 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2024

Plunging region emission in the X-ray binary MAXI J0637430

Andrew Mummery, Jiachen Jiang, Andrew Fabian

On the second of November 2019 the black hole X-ray binary MAXI J0637430 went into outburst, at the start of which it was observed in a thermal ``disc-dominated'' state. High ph…

astro-ph.HE2024

The Origin of the X-ray Emission from the Non-Starburst Gas-Rich Luminous Infrared Galaxies Arp 302

Jiachen Jiang, William Baker, Andrew Young +1

We present an analysis of the XMM-Newton observation of luminous infrared merging galaxies Arp 302 and a joint re-analysis of its Chandra observation. In particular, we focus on th…

astro-ph.HE202412 cited

Towards more accurate synthetic reflection spectra: improving the calculations of returning radiation

Temurbek Mirzaev, Shafqat Riaz, Askar B. Abdikamalov +6

We present a new model to calculate reflection spectra of thin accretion disks in Kerr spacetimes. Our model includes the effect of returning radiation, which is the radiation that…

astro-ph.HE20231 cited

The High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black Holes

Riley Connors, John Tomsick, Paul Draghis +20

Accretion is a universal astrophysical process that plays a key role in cosmic history, from the epoch of reionization to galaxy and stellar formation and evolution. Accreting stel…

astro-ph.HE202310 cited

An XMM-Newton Study of Six Narrow-Line Seyfert 1 Galaxies at z = 0.35--0.92

Zhibo Yu, Jiachen Jiang, Cosimo Bambi +5

We report a detailed analysis of the XMM-Newton spectra of six Narrow-Line Seyfert 1 (NLS1) galaxies at redshift z = 0.35--0.92. Compared with the NLS1s at lower redshift in the pr…

astro-ph.HE202312 cited

Reflection and timing study of the transient black hole X-ray binary MAXI J1803-298 with NuSTAR

Benjamin M. Coughenour, John A. Tomsick, Guglielmo Mastroserio +9

The transient black hole X-ray binary MAXI J1803-298 was discovered on 2021 May 1, as it went into outburst from a quiescent state. As the source rose in flux it showed periodic ab…