activity
20162026
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 15.1k across the 90 of their papers we have counts for

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astro-ph.HE2026

Broadband multiwavelength properties of the archetypal blazar 3C 279 during the 2017 Event Horizon Telescope campaign

G. Principe, J. C. Algaba, E. Aviano +529

The archetypal blazar 3C 279 hosts a prominent relativistic jet and exhibits strong broadband variability across the electromagnetic spectrum. In April 2017, the Event Horizon Tele…

astro-ph.HE2026

Non-thermal X-ray Emission from Merging Massive Black Hole Binaries

Luke Krauth, Jordy Davelaar

Recent hydrodynamical simulations have identified a disappearing thermal X-ray signature in massive black hole binaries (MBHBs) embedded in circumbinary disks, arising from the tid…

astro-ph.HE2026★ 1 cited

Ring Asymmetry and Spin in M87*

Vadim Bernshteyn, Nicholas S. Conroy, Michi Bauböck +263

Event Horizon Telescope (EHT) images of the supermassive black hole M87* depict an asymmetric ring of emission. General relativistic magnetohydrodynamic (GRMHD) models of M87* and…

astro-ph.HE2025

Self-lensing flares from black hole binaries V: systematic searches in LSST

Kevin Park, Zoltan Haiman, Chengcheng Xin +3

The Vera C. Rubin Observatory has now seen first light, and over a 10 year duration, LSST is projected to catalogue tens of millions of quasars, many of which are expected to be as…

astro-ph.HE2025★ 4 cited

Probing jet base emission of M87* with the 2021 Event Horizon Telescope observations

Saurabh, Hendrik Müller, Sebastiano D. von Fellenberg +282

We investigate the presence and spatial characteristics of the jet base emission in M87* at 230 GHz, enabled by the enhanced uv coverage in the 2021 Event Horizon Telescope (EHT) o…

astro-ph.HE2025

Fill the gaps: continuous in time interpolation of fluid dynamical simulations

Jonas Pronk, Oliver Porth, Jordy Davelaar

Flexible and accurate interpolation schemes using machine learning could be of great benefit for many use-cases in numerical simulations and post-processing, such as temporal upsam…

astro-ph.HE2025

Changing-Look AGN Powered By Disk Tearing

Nicholas Kaaz, Matthew Liska, Charlotte Ward +1

Changing-look active galactic nuclei (CLAGN) feature order-of-magnitude variability in both the continuum and broad line luminosities on months-to-years long timescales, and are cu…

astro-ph.HE2025★ 4 cited

Origin of the ring ellipticity in the black hole images of M87*

Rohan Dahale, Ilje Cho, Kotaro Moriyama +273

We investigate the origin of the elliptical ring structure observed in the images of the supermassive black hole M87*, aiming to disentangle contributions from gravitational, astro…

astro-ph.HE2025★ 1 cited

A search for periodic AGN variability in Data Release 3

Pablo Huijse, Jordy Davelaar, Joris De Ridder +2

Supermassive black hole binaries (SMBHB) are expected to produce periodic modulations in active galactic nuclei (AGN) light curves, but distinguishing such signals from stochastic…

astro-ph.HE2025

Modeling of lightcurves from reconnection-powered very high energy flares from M87*

Siddhant Solanki, Jordy Davelaar, Bart Ripperda +1

The black hole at the center of M87 is observed to flare regularly in the very high energy (VHE) band, with photon energies GeV. The rapid variability, which can be a…

astro-ph.HE2025

Novel Polarimetric Analysis of Near Horizon Flaring Episodes in M87* in Millimeter Wavelength

Razieh Emami, Matthew Liska, Koushik Chatterjee +15

Recent multi-wavelength observations of M87* \citep{2024A&A...692A.140A} revealed a high-energy -ray flare without a corresponding millimeter counterpart. We present a theoretic…

astro-ph.HE2025★ 2 cited

Thermal X-ray signatures in late-stage unequal-mass massive black hole binary mergers

Luke Major Krauth, Jordy Davelaar, Zoltán Haiman +3

The multi-messenger combination of gravitational waves (GWs) from merging massive black hole binaries (MBHBs) and the electromagnetic (EM) counterpart from the surrounding circumbi…

astro-ph.HE2025★ 10 cited

The putative center in NGC 1052

Anne-Kathrin Baczko, Matthias Kadler, Eduardo Ros +284

Many active galaxies harbor powerful relativistic jets, however, the detailed mechanisms of their formation and acceleration remain poorly understood. To investigate the area of je…

astro-ph.HE2025★ 13 cited

A multi-frequency study of sub-parsec jets with the Event Horizon Telescope

Jan Röder, Maciek Wielgus, Andrei P. Lobanov +287

The 2017 observing campaign of the Event Horizon Telescope (EHT) delivered the first very long baseline interferometry (VLBI) images at the observing frequency of 230 GHz, leading…

astro-ph.HE2024★ 2 cited

Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations

Pushpita Das, Tuomo Salmi, Jordy Davelaar +2

The pulsed X-ray emission from the neutron star surface acts as a window to study the state of matter in the neutron star interior. For accreting millisecond pulsars, the surface X…

astro-ph.HE2024★ 19 cited

Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona

Navin Sridhar, Bart Ripperda, Lorenzo Sironi +2

Using two-dimensional general relativistic resistive magnetohydrodynamic simulations, we investigate the properties of the sheath separating the black hole jet from the surrounding…

astro-ph.HE2024

Machine- and deep-learning-driven angular momentum inference from BHEX observations of the photon ring

Joseph R. Farah, Jordy Davelaar, Daniel Palumbo +2

The photon ring is an important probe of black hole (BH) properties and will be resolved by the Black Hole Explorer (BHEX) for the first time. However, extraction of black ho…

astro-ph.HE2024★ 2 cited

Machine-Learning Characterization of Intermittency in Relativistic Pair Plasma Turbulence: Single and Double Sheet Structures

Trung Ha, Joonas Nättilä, Jordy Davelaar +1

The physics of turbulence in magnetized plasmas remains an unresolved problem. The most poorly understood aspect is intermittency -- spatio-temporal fluctuations superimposed on th…

astro-ph.HE2024

Self-lensing flares from black hole binaries IV: the number of detectable shadows

Kevin Park, Chengcheng Xin, Jordy Davelaar +1

Sub-parsec supermassive black hole (SMBH) binaries are expected to be common in active galactic nuclei (AGN), as a result of the hierarchical build-up of galaxies via mergers. Whil…

astro-ph.HE2024

MLody -- Deep Learning Generated Polarized Synchrotron Coefficients

Jordy Davelaar

Polarized synchrotron emission is a fundamental process in high-energy astrophysics, particularly in the environments around black holes and pulsars. Accurate modeling of this emis…

astro-ph.HE2024

Relativistic Binary Precession: Impact on Eccentric Binary Accretion and Multi-Messenger Astronomy

Stanislav DeLaurentiis, Zoltan Haiman, John Ryan Westernacher-Schneider +4

Recent hydrodynamical simulations have shown that circumbinary gas disks drive the orbits of binary black holes to become eccentric, even when general relativistic corrections to t…

astro-ph.HE2024★ 34 cited

Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring Episode

J. C. Algaba, M. Balokovic, S. Chandra +738

The nearby elliptical galaxy M87 contains one of the only two supermassive black holes whose emission surrounding the event horizon has been imaged by the Event Horizon Telescope (…

astro-ph.HE2024★ 7 cited

Imaging the event horizon of M87* from space on different timescales

Anastasia Shlentsova, Freek Roelofs, Sara Issaoun +2

The concept of a new space very long baseline interferometry system named the Event Horizon Imager (EHI) has been proposed to dramatically improve black hole imaging and provide pr…

astro-ph.HE2024★ 26 cited

Ordered magnetic fields around the 3C 84 central black hole

G. F. Paraschos, J. -Y. Kim, M. Wielgus +279

3C84 is a nearby radio source with a complex total intensity structure, showing linear polarisation and spectral patterns. A detailed investigation of the central engine region nec…