activity
20112026
most citedImproved Reflection Models of Black-Hole Accretion Disks: Treating the Angular Distribution of X-rays

715 citations · 3.7k across the 78 of their papers we have counts for

collaborators

80 papers

astro-ph.HE2026

Flux Dependence of the 1\,keV Soft X-ray Feature in SAX J1808.4-3658 with \textit{NICER}

Katherine Bruce, Anne M. Lohfink, Jaiverdhan Chauhan +3

We present a systematic X-ray spectral analysis of the 2019 and 2022 outbursts of the accreting millisecond pulsar SAX J1808.4-3658 with extit{NICER} with a particular emphasis on…

astro-ph.HE2026

PACHA: Probing AGN Coronae with High-redshift AGN

Xiurui Zhao, Elias Kammoun, Marco Ajello +18

The X-ray emission of active galactic nuclei (AGN) is generally attributed to inverse Compton scattering of accretion-disk photons by hot electrons in a compact corona. In local AG…

astro-ph.GA2025

Chandra and HST Observations of Radio-Selected (Wandering) Massive Black Hole Candidates in Dwarf Galaxies

Megan R. Sturm, Amy E. Reines, Anne M. Lohfink +6

We present Chandra X-ray Observatory and Hubble Space Telescope (HST) follow-up observations of 12 dwarf galaxies from Reines et al. (2020) that are potential hosts of radio-select…

astro-ph.HE2025

Establishing a Connection Between the Jet and the Corona in Black Hole Low Mass X-Ray Binaries

Eric Davidson, Jaiverdhan Chauhan, Anne Lohfink +3

Low-mass black hole X-ray Binaries (LMXBs) undergo outbursts, during which their brightness increases greatly for timescales of months. The X-ray accretion and radio jet properties…

astro-ph.HE2025

QPO signatures of disk restoration after type-I X-ray bursts from 4U~1636536

Suchismito Chattopadhyay, Jaiverdhan Chauhan, Ranjeev Misra +4

Type--I thermonuclear bursts (TNBs) from neutron star low-mass X-ray binaries (NS LMXBs) originate on the neutron star's surface from the unstable burning of the accreted material.…

astro-ph.HE2025★ 4 cited

Probing thermonuclear bursts and X-ray reflection features in Aql X-1 during 2024 outburst

Manoj Mandal, Sabyasachi Pal, G. K. Jaisawal +3

We report the broadband timing and spectral properties of the neutron star low-mass X-ray binary Aql X-1 during the 2024 outburst with NICER, NuSTAR, and Swift observatories. We de…

astro-ph.HE2025

A new independent look at the galactic black hole low-mass X-ray binary distribution

Youssef Abdulghani, Anne M Lohfink, Jaiverdhan Chauhan

Investigations of the Galactic black hole low-mass X-ray binaries (BH-LMXBs) offer valuable insights into the elusive black hole population in the Milky Way. Motivated by recent te…

astro-ph.HE2024★ 7 cited

A Dependable Distance Estimator to Black Hole Low-Mass X-ray Binaries

Youssef Abdulghani, Anne M Lohfink, Jaiverdhan Chauhan

Black Hole Low Mass X-ray Binaries (BH-LMXBs) are excellent observational laboratories for studying many open questions in accretion physics. However, determining the physical prop…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nuclei

E. Kammoun, A. M. Lohfink, M. Masterson +28

The hard X-ray emission in active galactic nuclei (AGN) and black hole X-ray binaries is thought to be produced by a hot cloud of electrons referred to as the corona. This emission…

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★ 20 cited

X-ray Reverberation Mapping of Ark 564 using Gaussian Process Regression

Collin D. Lewin, Erin Kara, Daniel R. Wilkins +15

Ark 564 is an extreme high-Eddington Narrow-line Seyfert 1 galaxy, known for being one of the brightest, most rapidly variable soft X-ray AGN, and for having one of the lowest temp…

astro-ph.HE2022★ 10 cited

The study of thermonuclear X-ray bursts in accreting millisecond pulsar MAXI J1816-195 with NuSTAR and NICER

Manoj Mandal, Sabyasachi Pal, Jaiverdhan Chauhan +2

The millisecond pulsar MAXI J1816-195 was recently discovered in an outburst by MAXI in 2022 May. We study different properties of the pulsar using data from NuSTAR and NICER obser…

astro-ph.HE2022★ 6 cited

Broadband spectral analysis of Mrk 926 using multi-epoch X-ray observations

S. Chalise, A. M. Lohfink, J. Chauhan +3

The X-ray spectra of some active galactic nuclei (AGN) show a soft X-ray excess, emission in excess to the extrapolated primary X-ray continuum below 2 keV. Recent studies have sho…

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.HE2021★ 6 cited

A Spectroscopic Angle on Central Engine Size Scales in Accreting Neutron Stars

Nicolas Trueba, J. M. Miller, A. C. Fabian +9

Analyses of absorption from disk winds and atmospheres in accreting compact objects typically treat the central emitting regions in these systems as point sources relative to the a…

astro-ph.HE2021★ 16 cited

The Inner Accretion Flow in the Resurgent Seyfert-1.2 AGN Mrk 817

J. M. Miller, Z. Zoghbi, M. T. Reynolds +10

Accretion disks and coronae around massive black holes have been studied extensively, and they are known to be coupled. Over a period of 30 years, however, the X-ray (coronal) flux…

astro-ph.HE2021★ 11 cited

Discovery of soft and hard X-ray time lags in low-mass AGNs

Labani Mallick, Daniel R. Wilkins, William N. Alston +5

The scaling relations between the black hole (BH) mass and soft lag properties for both active galactic nuclei (AGNs) and BH X-ray binaries (BHXRBs) suggest the same underlying phy…

astro-ph.HE2020★ 152 cited

Towards precision measurements of accreting black holes using X-ray reflection spectroscopy

Cosimo Bambi, Laura W. Brenneman, Thomas Dauser +14

Relativistic reflection features are commonly observed in the X-ray spectra of accreting black holes. In the presence of high quality data and with the correct astrophysical model,…

astro-ph.HE2020★ 30 cited

A hard look at local, optically-selected, obscured Seyfert galaxies

E. S. Kammoun, J. M. Miller, M. Koss +11

We study the X-ray spectra of a sample of 19 obscured, optically-selected Seyfert galaxies (Sy 1.8, 1.9 and 2) in the local universe (~Mpc), drawn from the CfA Seyfert…

astro-ph.GA2020★ 105 cited

Intensive disc-reverberation mapping of Fairall 9: 1st year of Swift & LCO monitoring

J. V. Hernández Santisteban, R. Edelson, K. Horne +33

We present results of time-series analysis of the first year of the Fairall 9 intensive disc-reverberation campaign. We used Swift and the Las Cumbres Observatory global telescope…

astro-ph.HE2020★ 16 cited

A Redshifted Inner Disk Atmosphere and Transient Absorbers in the Ultra-Compact Neutron Star X-ray Binary 4U 1916-053

Nicolas Trueba, J. M. Miller, A. C. Fabian +8

The very small accretion disks in ultra-compact X-ray binaries (UCXBs) are special laboratories in which to study disk accretion and outflows. We report on three sets of new (250 k…

astro-ph.HE2020★ 4 cited

Broad-band X-ray observation of broad-line radio galaxy 3C 109

Sulov Chalise, Anne M. Lohfink, Erin Kara +1

We present a study of the central engine in the broad-line radio galaxy 3C 109. To investigate the immediate surrounding of this accreting, supermassive black hole, we perform a mu…

astro-ph.HE2020★ 100 cited

A dynamic black hole corona in an active galaxy through X-ray reverberation mapping

William N. Alston, Andrew C. Fabian, Erin Kara +18

X-ray reverberation echoes are assumed to be produced in the strongly distorted spacetime around accreting supermassive black holes. This signal allows us to spatially map the geom…

astro-ph.HE2019★ 6 cited

X-ray spectral and flux variability of the microquasar GRS 1758-258 on timescales from weeks to years

Maria Hirsch, Katja Pottschmidt, David M. Smith +12

We present the spectral and timing evolution of the persistent black hole X-ray binary GRS 1758-258 based on almost 12 years of observations using the Rossi X-ray Timing Explorer P…