activity
19952023
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 41.1k across the 542 of their papers we have counts for

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Showing 2019 · astro-ph.HEShow all

22 papers · 2 filters

astro-ph.HE2019★ 20 cited

A NuSTAR View of GRS 1716249 in the Hard and Intermediate States

Jiachen Jiang, Felix Fürst, Dominic J. Walton +2

We present a detailed analysis of the spectral properties of the black hole transient GRS 1716-249, based on the archival Swift and NuSTAR observations taken during the outburst of…

astro-ph.HE2019

Lessons learned from 19 years of high-resolution X-ray spectroscopy of galaxy clusters with RGS

C. Pinto, A. C. Fabian, J. S. Sanders +1

The intracluster medium (ICM) contains the vast majority of the baryonic matter in galaxy clusters and is heated to X-ray radiating temperatures. X-ray spectroscopy is therefore a…

astro-ph.HE2019★ 24 cited

Discovery of a soft X-ray lag in the Ultraluminous X-ray Source NGC 1313 X-1

E. Kara, C. Pinto, D. J. Walton +14

Ultraluminous X-ray Sources (ULXs) provide a unique opportunities to probe the geometry and energetics of super-Eddington accretion. The radiative processes involved in super-Eddin…

astro-ph.HE2019

Astrophysical Black Holes

Andrew C. Fabian, Anthony N. Lasenby

Black holes are a common feature of the Universe. They are observed as stellar mass black holes spread throughout galaxies and as supermassive objects in their centres. Observation…

astro-ph.HE2019★ 52 cited

The Unusual Broadband X-ray Spectral Variability of NGC 1313 X-1 seen with XMMNewton, Chandra and NuSTAR

D. J. Walton, C. Pinto, M. Nowak +19

We present results from the major coordinated X-ray observing program on the ULX NGC 1313 X-1 performed in 2017, combining -, and , focusing on the e…

astro-ph.HE2019★ 50 cited

XMM-Newton Campaign On Ultraluminous X-ray Source NGC 1313 X-1: Wind vs. State Variability

C. Pinto, D. J. Walton, E. Kara +12

Most ultraluminous X-ray sources (ULXs) are thought to be powered by neutron stars and black holes accreting beyond the Eddington limit. If the compact object is a black hole or a…

astro-ph.HE2019★ 41 cited

X-ray Observations of Luminous Dusty Quasars at z > 2

G. B. Lansbury, M. Banerji, A. C. Fabian +1

We present new X-ray observations of luminous heavily dust-reddened quasars (HRQs) selected from infrared sky surveys. HRQs appear to be a dominant population at high redshifts and…

astro-ph.HE2019★ 41 cited

An evolving broad iron line from the first Galactic ultraluminous X-ray pulsar Swift J0243.6+6124

Gaurava K. Jaisawal, Colleen A. Wilson-Hodge, Andrew C. Fabian +15

We present a spectral study of the ultraluminous Be/X-ray transient pulsar Swift J0243.6+6124 using Neutron Star Interior Composition Explorer (NICER) observations during the syste…

astro-ph.HE2019★ 107 cited

MAXI J1820+070 with NuSTAR I. An increase in variability frequency but a stable reflection spectrum: coronal properties and implications for the inner disc in black hole binaries

D. J. K. Buisson, A. C. Fabian, D. Barret +10

MAXI J1820+070 (optical counterpart ASASSN-18ey) is a black hole candidate discovered through its recent very bright outburst. The low extinction column and long duration at high f…

astro-ph.HE2019★ 129 cited

High Density Reflection Spectroscopy: II. the Density of the Inner Black Hole Accretion Disc in AGN

Jiachen Jiang, Andrew C. Fabian, Thomas Dauser +7

We present a high density disc reflection spectral analysis of a sample of 17 Seyfert 1 galaxies to study the inner disc densities at different black hole mass scales and accretion…

astro-ph.HE2019★ 47 cited

The 2017 Failed Outburst of GX 339-4: Relativistic X-ray Reflection near the Black Hole Revealed by NuSTAR and Swift Spectroscopy

Javier A. García, John A. Tomsick, Navin Sridhar +12

We report on the spectroscopic analysis of the black hole binary GX 339-4 during its recent 2017-2018 outburst, observed simultaneously by the Swift and NuSTAR observatories. Altho…

astro-ph.HE2019★ 14 cited

Observations of the Ultra-compact X-ray Binary 4U 1543-624 in Outburst with NICER, INTEGRAL, Swift, and ATCA

R. M. Ludlam, L. Shishkovsky, P. M. Bult +17

We report on X-ray and radio observations of the ultra-compact X-ray binary 4U 1543-624 taken in August 2017 during an enhanced accretion episode. We obtained NICER monitoring of t…

astro-ph.HE2019★ 3 cited

The X-ray Coronae of two massive galaxies in the core of the Perseus cluster

N. Arakawa, A. C. Fabian, S. A. Walker

We study the X-ray properties of two elliptical galaxies, NGC 1270 and NGC 1272, in the core of the Perseus cluster with deep Chandra observations. Both galaxies have central super…

astro-ph.HE2019★ 3 cited

Supermassive Black Hole Feedback

Mateusz Ruszkowski, Daisuke Nagai, Irina Zhuravleva +23

Understanding the processes that drive galaxy formation and shape the observed properties of galaxies is one of the most interesting and challenging frontier problems of modern ast…

astro-ph.HE2019

Probing the Black Hole Engine with Measurements of the Relativistic X-ray Reflection Component

Javier A. García, Matteo Bachetti, David R. Ballantyne +21

Over the last decades X-ray spectroscopy has proven to be a powerful tool for the estimation of black hole spin and several other key parameters in dozens of AGN and black hole X-r…

astro-ph.HE2019★ 5 cited

The Advanced X-ray Imaging Satellite

Richard F. Mushotzky, James Aird, Amy J. Barger +41

Much of the baryonic matter in the Universe, including the most active and luminous sources, are best studied in the X-ray band. Key advances in X-ray optics and detectors have pav…

astro-ph.HE2019★ 3 cited

Probing the Physical Properties of the Corona in Accreting Black Holes

Nikita Kamraj, Andrew Fabian, Anne Lohfink +3

The corona is a key component of most luminous accreting black holes, carrying 5 - 30 % of the power and in non-jetted Active Galactic Nuclei (AGN), creating all the X-ray emission…

astro-ph.HE2019★ 21 cited

Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups

Haonan Liu, Ciro Pinto, Andrew C. Fabian +2

We present a spectral analysis of cool and cooling gas in 45 cool-core clusters and groups of galaxies obtained from Reflection Grating Spectrometer (RGS) XMM- observations…

astro-ph.HE2019★ 50 cited

Evidence for an emerging disc wind and collimated outflow during an X-ray flare in the narrow-line Seyfert 1 galaxy Mrk 335

L. C. Gallo, A. G. Gonzalez, S. G. H. Waddell +13

A triggered 140 ks XMM-Newton observation of the narrow-line Seyfert 1 (NLS1) Mrk 335 in December 2015 caught the active galaxy at its lowest X-ray flux since 2007. The NLS1 is rel…

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.HE2019★ 278 cited

The corona contracts in a black-hole transient

E. Kara, J. F. Steiner, A. C. Fabian +11

The geometry of the accretion flow around stellar-mass black holes can change on timescales of days to months. When a black hole emerges from quiescence (that is, it "turns on" aft…

astro-ph.HE2019★ 87 cited

High Density Reflection Spectroscopy I. A case study of GX~339-4

Jiachen Jiang, Andrew C. Fabian, Jingyi Wang +5

We present a broad band spectral analysis of the black hole binary GX~339-4 with NuSTAR and Swift using high density reflection model. The observations were taken when the source w…