activity
20082026
most citedA new relativistic component of the accretion disk wind in PDS 456

65 citations · 123 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

The Geometry of Ultra-Fast Outflows Probed by Soft X-ray Variability in PDS 456

Riki Sato, Kouichi Hagino, Toshiya Iwata +20

Constraining the location and geometry of ultra-fast outflows (UFOs) is essential for identifying where they are launched and how they are accelerated. We investigate the soft X-ra…

astro-ph.HE2026

Resolving the Multiple Component Outflows in PG 1211+143: II. The Soft X-ray View of the Ultra Fast Outflow

James Reeves, Valentina Braito, Misaki Mizumoto +16

The nearby quasar, PG 1211+143, has one of the prototype examples of an ultra fast outflow (UFO), as seen in several past XMM-Newton and Chandra observations. In December 2024, PG…

astro-ph.GA2025

The dynamic central environment of NGC 3516 revealed by XRISM

Anna Juráňová, Erin Kara, Ehud Behar +15

We present a detailed, time-resolved analysis of the Fe K band of the Seyfert 1.5 galaxy NGC 3516 observed with XRISM. The 249 ks observation spanning 310 ks in elapsed time…

astro-ph.HE2025

Resolving the Multiple Component Outflows in PG 1211+143: I. The Fe-K Absorption Structure and UFO Forest

Misaki Mizumoto, James N. Reeves, Valentina Braito +15

We present the initial high-resolution X-ray spectroscopic observations of the Fe-K absorption structure in the luminous nearby quasar PG 1211+143, utilizing the X-ray Imaging and…

astro-ph.HE2025★ 1 cited

A possible two-fold scenario for the disc-corona of the luminous AGN 1H 0419--577: a high-density disc or a warm corona

Delphine Porquet, James N. Reeves, Valentina Braito

[abridged] 1H 0419-577 is a highly-accreting, luminous BLS1 AGN. This study aims to characterise its disc-corona system using, for the first time, simultaneous XMM-Newton and NuSTA…

astro-ph.HE2025★ 11 cited

Unraveling the structure of the stratified ultra-fast outflows in PDS 456 with XRISM

Yerong Xu, Luigi C. Gallo, Kouichi Hagino +18

Multiple clumpy wind components () in the luminous quasar PDS 456 have recently been resolved by XRISM in the Fe-K band for the first time. In this paper, we i…

astro-ph.HE2020★ 6 cited

Modelling X-ray RMS spectra II: the ultra-fast outflow of PDS 456

L. Härer, M. L. Parker, A. Joyce +6

We present an improved model for excess variance spectra describing ultra-fast outflows and successfully apply it to the luminous (L ~ 10^47 erg/s) low-redshift (z = 0.184) quasar…

astro-ph.HE2018★ 65 cited

A new relativistic component of the accretion disk wind in PDS 456

James Reeves, Valentina Braito, Emanuele Nardini +3

Past X-ray observations of the nearby luminous quasar PDS 456 (at ) have revealed a wide angle accretion disk wind (Nardini et al. 2015), with an outflow velocity of $\sim…

astro-ph.GA2012

The Suzaku view of highly-ionised outflows in AGN

J. A. Gofford, J. N. Reeves, V. Braito +1

We are conducting a systematic study of highly-ionised outflows in AGN using archival Suzaku data. To date we have analysed 59 observations of 45 AGN using a combined energy-intens…

astro-ph2008★ 40 cited

X-Ray Spectral Variability of the Seyfert Galaxy NGC 4051 Observed with Suzaku

Y. Terashima, L. C. Gallo, H. Inoue +13

We report results from a Suzaku observation of the narrow-line Seyfert 1 NGC 4051. During our observation, large amplitude rapid variability is seen and the averaged 2--10 keV flux…