activity
20212026
most citedDisk, Corona, Jet Connection in the Intermediate State of MAXI J1820+070 Revealed by NICER Spectral-Timing Analysis

96 citations · 391 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.IM2026

High performance Stingray

Eleonora Veronica Lai, Matteo Bachetti, Maura Pilia +4

X-ray astrophysical objects show variability on a wide range of timescales, i.e. from fractions of second to years. The open-source Python library stingray is able to perform time…

astro-ph.IM2026

Emulation of non-linear 1D spectral models: relativistic X-ray reflection

Benjamin J. Ricketts, Tin Hadži Veljković, Daniela Huppenkothen +4

The use of machine learning techniques to approximate computationally expensive models has become increasingly prevalent in a wide variety of fields within astronomy. We discuss th…

astro-ph.HE2025

X-ray reverberation black hole mass and distance estimates of Cygnus X-1

Patrick O'Neill, Adam Ingram, Edward Nathan +4

We fit X-ray reverberation models to Rossi X-ray Timing Explorer data from the X-ray binary Cygnus X-1 in its hard state to yield estimates for the black hole mass and the distance…

astro-ph.HE2024★ 1 cited

RTFAST-Spectra: Emulation of X-ray reverberation mapping for active galactic nuclei

Benjamin Ricketts, Daniela Huppenkothen, Matteo Lucchini +4

Bayesian analysis has begun to be more widely adopted in X-ray spectroscopy, but it has largely been constrained to relatively simple physical models due to limitations in X-ray mo…

astro-ph.HE2024

Characterizing the Broadband Reflection Spectrum of MAXI J1803-298 During its 2021 Outburst with NuSTAR and NICER

Oluwashina Adegoke, Javier Garcia, Riley Connors +12

MAXI J1803-298 is a transient black hole candidate discovered in May of 2021 during an outburst that lasted several months. Multiple X-ray observations reveal recurring "dipping" i…

astro-ph.HE2024★ 8 cited

Proof of principle X-ray reflection mass measurement of the black hole in H1743-322

Edward Nathan, Adam Ingram, James F. Steiner +9

The black hole X-ray binary H1743-322 lies in a region of the Galaxy with high extinction, and therefore it has not been possible to make a dynamical mass measurement. In this pape…

astro-ph.HE2024

Correlated mid-infrared and X-ray outbursts in black hole X-ray binaries: A new route to discovery in infrared surveys

Chris John, Kishalay De, Matteo Lucchini +5

The mid-infrared (MIR; m) bands offer a unique window into understanding accretion and its interplay with jet formation in Galactic black hole X-ray binaries (BHXRB…

astro-ph.HE2024★ 20 cited

Long term variability of Cygnus X-1. VIII. A spectral-timing look at low energies with NICER

Ole König, Guglielmo Mastroserio, Thomas Dauser +19

The Neutron Star Interior Composition Explorer (NICER) monitoring campaign of Cyg X-1 allows us to study its spectral-timing behavior at energies keV across all states. The…

astro-ph.HE2024

Highly-coherent quasi-periodic oscillations in the 'heartbeat' black hole X-ray binary IGR J17091-3624

Jingyi Wang, Erin Kara, Jeroen Homan +13

IGR J17091-3624 is a black hole X-ray binary (BHXB), often referred to as the 'twin' of GRS 1915+105 because it is the only other known BHXB that can show exotic 'heartbeat'-like v…

astro-ph.HE2024

The 2022 Outburst of IGR J17091-3624: Connecting the exotic GRS 1915+105 to standard black hole X-ray binaries

Jingyi Wang, Erin Kara, Javier A. García +13

While the standard X-ray variability of black hole X-ray binaries (BHXBs) is stochastic and noisy, there are two known BHXBs that exhibit exotic `heartbeat'-like variability in the…

astro-ph.HE2023★ 23 cited

Chasing the break: Tracing the full evolution of a black hole X-ray binary jet with multi-wavelength spectral modeling

Constanza Echiburú-Trujillo, Alexandra J. Tetarenko, Daryl Haggard +35

Black hole X-ray binaries (BH XRBs) are ideal targets to study the connection between accretion inflow and jet outflow. Here we present quasi-simultaneous, multi-wavelength observa…

astro-ph.HE2023

Variability as a predictor for the hard-to-soft state transition in GX 339-4

Matteo Lucchini, Marina Ten Have, Jingyi Wang +17

During the outbursts of black hole X-ray binaries (BHXRBs), their accretion flows transition through several states. The source luminosity rises in the hard state, dominated by non…

astro-ph.HE2023★ 21 cited

Investigating the impact of vertically extended coronae on X-ray reverberation mapping

Matteo Lucchini, Guglielmo Mastroserio, Jingyi Wang +9

Accreting black holes commonly exhibit hard X-ray emission, originating from a region of hot plasma near the central engine referred to as the corona. The origin and geometry of th…

astro-ph.HE2023★ 6 cited

The peculiar variable X-ray spectrum of the active galactic nucleus PKS 2005-489

Owen Chase, Felicia McBride, Andrea Gokus +4

PKS 2005-489 is a well-known, bright southern BL Lac object that has been detected up to TeV energies. In a low-flux state it exhibits the expected multiwavelength double-peaked sp…

astro-ph.HE2023★ 7 cited

Unusual Hard X-ray Flares Caught in NICER Monitoring of the Binary Supermassive Black Hole Candidate AT2019cuk/Tick Tock/SDSS J1430+2303

Megan Masterson, Erin Kara, Dheeraj R. Pasham +17

The nuclear transient AT2019cuk/Tick Tock/SDSS J1430+2303 has been suggested to harbor a supermassive black hole (SMBH) binary near coalescence. We report results from high-cadence…

astro-ph.HE2022★ 82 cited

The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole

Dheeraj R. Pasham, Matteo Lucchini, Tanmoy Laskar +63

A black hole can launch a powerful relativistic jet after it tidally disrupts a star. If this jet fortuitously aligns with our line of sight, the overall brightness is Doppler boos…

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★ 62 cited

The NICER "Reverberation Machine": A Systematic Study of Time Lags in Black Hole X-Ray Binaries

Jingyi Wang, Erin Kara, Matteo Lucchini +12

We perform the first systematic search of all NICER archival observations of black hole (and candidate) low-mass X-ray binaries for signatures of reverberation. Reverberation lags…

astro-ph.HE2021★ 8 cited

On measuring the Hubble constant with X-ray reverberation mapping of active galactic nuclei

Adam Ingram, Guglielmo Mastroserio, Michiel van der Klis +8

We show that X-ray reverberation mapping can be used to measure the distance to type 1 active galactic nuclei (AGNs). This is because X-ray photons originally emitted from the `cor…

astro-ph.HE2021★ 37 cited

Modelling correlated variability in accreting black holes: the effect of high density and variable ionisation on reverberation lags

Guglielmo Mastroserio, Adam Ingram, Jingyi Wang +9

We present a new release of the RELTRANS model to fit the complex cross-spectrum of accreting black holes as a function of energy. The model accounts for continuum lags and reverbe…

astro-ph.HE2021★ 96 cited

Disk, Corona, Jet Connection in the Intermediate State of MAXI J1820+070 Revealed by NICER Spectral-Timing Analysis

Jingyi Wang, Guglielmo Mastroserio, Erin Kara +14

We analyze 5 epochs of NICER data of the black hole X-ray binary MAXI J1820+070 during the bright hard-to-soft state transition in its 2018 outburst with both reflection spectrosco…