activity
20132025
most citedHigh-Density Effects in X-ray Reflection Models from Accretion Disks

184 citations · 2.2k across the 43 of their papers we have counts for

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40 papers · 1 filter

astro-ph.HE2025

The Broadband View of the Bare Seyfert PG 1426+015: Relativistic Reflection, the Soft Excess and the Importance of Oxygen

D. J. Walton, A. Madathil-Pottayil, P. Kosec +8

We present results from a deep, coordinated - + observation of the type 1 Seyfert PG 1426+015, a source of particular interest as the most massive reverberati…

astro-ph.HE2023

The RS Oph outburst of 2021 monitored in X-rays with NICER

Marina Orio, Keith Gendreau, Morgan Giese +19

The 2021 outburst of the symbiotic recurrent nova RS Oph was monitored with the Neutron Star Interior Composition Explorer Mission (NICER) in the 0.2-12 keV range from day one afte…

astro-ph.HE2023★ 5 cited

Stellar wind variability in Cygnus X-1 from high-resolution excess variance spectroscopy with Chandra

Lucia K. Härer, Michael L. Parker, Ileyk El Mellah +5

Stellar winds of massive stars are known to be driven by line absorption of UV photons, a mechanism which is prone to instabilities, causing the wind to be clumpy. The clumpy struc…

astro-ph.HE2023★ 40 cited

UV/Optical disk reverberation lags despite a faint X-ray corona in the AGN Mrk 335

Erin Kara, Aaron J. Barth, Edward M. Cackett +37

We present the first results from a 100-day Swift, NICER and ground-based X-ray/UV/optical reverberation mapping campaign of the Narrow-Line Seyfert 1 Mrk 335, when it was in an un…

astro-ph.HE2022★ 7 cited

Physics Beyond the Standard Model with Future X-ray Observatories: Projected Constraints on Very-Light Axion-Like Particles with and

Júlia Sisk-Reynés, Christopher S. Reynolds, Michael L. Parker +2

Axion-Like Particles (ALPs) are well-motivated extensions of the Standard Model of Particle Physics and a generic prediction of some string theories. X-ray observations of bright A…

astro-ph.HE2022★ 7 cited

X-ray spectral and timing analysis of the Compton Thick Seyfert 2 galaxy NGC 1068

Indrani Pal, C. S. Stalin, M. L. Parker +2

We present the timing and spectral analysis of the Compton Thick Seyfert 2 active galactic nuclei NGC 1068 observed using {\it NuSTAR} and {\it XMM-Newton}. In this work for the fi…

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★ 10 cited

The long-stable hard state of XTE J1752-223 and the disk truncation dilemma

Riley M. T. Connors, Javier A. Garcia, John Tomsick +10

The degree to which the thin accretion disks of black hole X-ray binaries are truncated during hard spectral states remains a contentious open question in black hole astrophysics.…

astro-ph.HE2022★ 17 cited

A New Emulated Monte Carlo Radiative Transfer Disk-Wind Model: X-Ray Accretion Disk-wind Emulator -- XRADE

G. A. Matzeu, M. Lieu, M. T. Costa +14

We present a new X-Ray Accretion Disk-wind Emulator (\textsc{xrade}) based on the 2.5D Monte Carlo radiative transfer code which provides a physically-motivated, self-consistent tr…

astro-ph.HE2022★ 9 cited

AGN X-ray Spectroscopy with Neural Networks

M. L. Parker, M. Lieu, G. A. Matzeu

We explore the possibility of using machine learning to estimate physical parameters directly from AGN X-ray spectra without needing computationally expensive spectral fitting. Spe…

astro-ph.HE2022★ 24 cited

High-density disc reflection spectroscopy of low-mass active galactic nuclei

L. Mallick, A. C. Fabian, J. A. García +13

The standard alpha-disc model predicts an anti-correlation between the density of the inner accretion disc and the black hole mass times square of the accretion rate, as seen in hi…

astro-ph.HE2022★ 25 cited

The X-ray Disk/Wind Degeneracy in AGN

M. L. Parker, G. A. Matzeu, J. H. Matthews +4

Relativistic Fe K emission lines from accretion disks and from disk winds encode key information about black holes, and their accretion and feedback mechanisms. We show that these…

astro-ph.HE2021★ 45 cited

Ionised Emission and Absorption in a Large Sample of Ultraluminous X-ray Sources

P. Kosec, C. Pinto, C. S. Reynolds +6

Most Ultraluminous X-ray sources (ULXs) are thought to be powered by super-Eddington accretion onto stellar-mass compact objects. Accretors in this extreme regime are naturally exp…

astro-ph.HE2021★ 32 cited

The nature of the extreme X-ray variability in the NLS1 1H 0707-495

M. L. Parker, W. N. Alston, L. Härer +11

We examine archival XMM-Newton data on the extremely variable narrow-line Seyfert 1 (NLS1) active galactic nucleus (AGN) 1H 0707-495. We construct fractional excess variance (Fvar)…

astro-ph.HE2020★ 15 cited

MAXI J1820+070 with NuSTAR II. Flaring during the hard to soft state transition with a long soft lag

D. J. K. Buisson, A. C. Fabian, P. Gandhi +6

We continue the analysis of NuSTAR data from the recent discovery outburst of MAXI J1820+070 (optical counterpart ASASSN-18ey), focussing on an observation including unusual flarin…

astro-ph.HE2020★ 29 cited

The first broadband X-ray view of the narrow line Seyfert 1 Ton S180

G. A. Matzeu, E. Nardini, M. L. Parker +15

We present joint \textit{XMM-Newton} and \textit{NuSTAR} observations of the `bare' narrow line Seyfert 1 Ton S180 (), carried out in 2016 and providing the first hard X-r…

astro-ph.HE2020

The Origin of X-ray Emission in the Gamma-ray emitting Narrow-Line Seyfert 1 1H 0323+342

Sergio A. Mundo, Erin Kara, Edward M. Cackett +7

We present the results of X-ray spectral and timing analyses of the closest gamma-ray emitting narrow-line Seyfert 1 (-NLS1) galaxy, 1H 0323+342. We use observations from a rece…

astro-ph.HE2019★ 58 cited

General Physical Properties of Gamma-ray Emitting Narrow-Line Seyfert 1 Galaxies

Vaidehi S. Paliya, M. L. Parker, J. Jiang +4

We present the results of a detailed multi-wavelength study of a sample of sixteen narrow-line Seyfert 1 (NLSy1) galaxies known in -rays so far. This includes a focused X-ray sp…

astro-ph.HE2018★ 23 cited

NuSTAR observations of Mrk 766: distinguishing reflection from absorption

D. J. K. Buisson, M. L. Parker, E. Kara +14

We present two new NuSTAR observations of the narrow line Seyfert 1 (NLS1) galaxy Mrk 766 and give constraints on the two scenarios previously proposed to explain its spectrum and…

astro-ph.HE2018★ 17 cited

X-ray spectral variability of blazars using principal component analysis

Dennis Gallant, Luigi C. Gallo, Michael L. Parker

Principal Component Analysis (PCA) is applied to a variety of blazars to examine X-ray spectral variability. Data from nine different objects are analysed in two ways: long-term, w…

astro-ph.HE2018★ 35 cited

A high-density relativistic reflection origin for the soft and hard X-ray excess emission from Mrk 1044

Labani Mallick, William N. Alston, Michael L. Parker +7

We present the first results from a detailed spectral-timing analysis of a long (130 ks) XMM-Newton observation and quasi-simultaneous NuSTAR and Swift observations of the hi…

astro-ph.HE2018★ 105 cited

The 1.5 Ms Observing Campaign on IRAS 13224-3809: X-ray Spectral Analysis I

J. Jiang, M. L. Parker, A. C. Fabian +16

We present a detailed spectral analysis of the recent 1.5\,Ms XMM-Newton observing campaign on the narrow line Seyfert 1 galaxy IRAS~132243809, taken simultaneously with 500\,ks…

astro-ph.HE2017★ 76 cited

A Hard Look at the Neutron Stars and Accretion Disks in 4U 1636-53, GX 17+2, and 4U 1705-44 with

R. M. Ludlam, J. M. Miller, M. Bachetti +9

We present observations of neutron star (NS) low-mass X-ray binaries: 4U 1636-53, GX 17+2, and 4U 1705-44. We observed 4U 1636-53 in the hard state, with an Eddingt…

astro-ph.HE2016★ 28 cited

A strongly truncated inner accretion disk in the Rapid Burster

J. van den Eijnden, T. Bagnoli, N. Degenaar +4

The neutron star (NS) low-mass X-ray binary (LMXB) the Rapid Burster (RB; MXB 1730-335) uniquely shows both Type-I and Type-II X-ray bursts. The origin of the latter is ill-underst…