First Sagittarius A* Event Horizon Telescope Results: VIII. Physical Interpretation of the Polarized Ring

First Sagittarius A* Event Horizon Telescope Results: VII. Polarization of the Ring

The Persistent Shadow of the Supermassive Black Hole of M87-I Observations, Calibration, Imaging and Analysis

Ordered Magnetic Fields Around the 3C 84 Central Black Hole

On the Comparison of AGN with GRMHD Simulations: II. M87

A search for pulsars around Sgr A* in the first Event Horizon Telescope dataset

First M87 Event Horizon Telescope Results. IX: Detection of Near-Horizon Circular Polarization

Polarimetric Geometric Modeling for mm-VLBI Observations of Black Holes

Comparison of Polarized Radiative Transfer Codes used by the EHT Collaboration

Accreting Primordial Black Holes and Dark Matter Candidates

The Event Horizon Telescope Image of the Quasar NRAO 530

Modeling Reconstructed Images of Jets Launched by SANE Super-Eddington Accretion Flows Around SMBHs with the ngEHT (v1) (v2)

Probing Plasma Composition with the Next Generation Event Horizon Telescope (ngEHT) (v1) (v2)

Tracing the Hotspot Motion Using the Next Generation Event Horizon Telescope (ngEHT) (v1) (v2)

Emission Modeling in the EHT-ngEHT Age (v1) (v2)

Unraveling Twisty Linear Polarization Morphologies in Black Hole Images (v1) (v2)

Jets from SANE Super-Eddington Accretion Disks: Morphology, Spectra and Their Potential as Targets for ngEHT (v1) (v2)

First Sagittarius A* Event Horizon Telescope Results. VI. Testing the Black Hole Metric

First Sagittarius A* Event Horizon Telescope Results. V. Testing Astrophysical Models of the Galactic Center Black Hole

First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology and Black Hole Mass

First Sagittarius A* Event Horizon Telescope Results. III. Imaging of the Galactic Center Supermassive Black Hole

First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing and Calibration

First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Black Hole in the Center of the Milky Way

Characterizing and Mitigating Intraday Variability: Reconstructing Source Structure in Accreting Black Holes with mm-VLBI

Selective Dynamical Imaging of Interferometric Data

A Universal Power-law Prescription for Variability from Synthetic Images of Black Hole Accretion Flows

The Variability of the Black-Hole Image in M87 at the Dynamical Timescale

Millimeter Light Curves of Sgr A* Observed during the 2017 Event Horizon Telescope Campaign

Positron Effects on Polarized Images and Spectra from Jet and Accretion Flow Models of M87 and Sgr A* (v1) (v2) (v3) (v4)

Event Horizon Telescope observations of the jet launching and collimation in Centaurus A

Constraints on black-hole charges with the 2017 EHT observations of M87*

Broadband Multi-Wavelength Properties of M87 During the 2017 Event Horizon Telescope Campaign

First Event Horizon Telescope Results. VIII. Magnetic Field Structure Near the Event Horizon

First Event Horizon Telescope Results. VII. Polarization of the Ring

Polarimetric Properties of Event Horizon Telescope Targets from ALMA

On the Comparison of AGN with GRMHD Simulations. I: Sgr A* (v1) (v2)

Determining the Composition of Relativistic Jets from Polarization Maps (v1) (v2)

A Quasi-Static Hyper-Resistive Model of UHE Cosmic Ray Acceleration by Magnetically Collimated Jets Created by AGN (v1) (v2)

Multiwavelength Observations of Relativistic Jets from General Relativistic Magnetohydrodynamic Simulations

The Future of Black Hole Astrophysics in the LIGO-VIRGO-LPF Era

Towards Multiwavelength Observations of Relativistic Jets from General Relativistic Magnetohydrodynamic Simulations (Stanford PhD Thesis)

Minute-Timescale >100MeV Gamma Ray Variability During the Giant Outburst of Quasar 3C 279 Observed by FERMI-LAT in June 2015

The Pauli Exclusion Principle at Strong Coupling – Holographic Matter and Momentum Space

TeV gamma rays from distant BL-Lacs and photon-paraphoton kinetic mixing

Grand Unification Scale Primordial Black Holes – Consequences and Constraints

Cover Story (view full-size image) M87 jet magnetic flux tubes are observed here at 15 GHz by the VLBA (courtesy of Kellermann, K.; et al.), possibly indicative of the magnetic Kelvin-Helmholtz instability. This pattern also appears in simulation models (Anantua et al. 2018) when the energy density of relativistic electrons in the radio jet does not decline with magnetic field strength at increasing radii from the black hole. With observation length scales over an order of magnitude greater than simulation scales, more remote processes such as coupling to the rotating interstellar medium may be responsible for the twisting flux tubes observed than in the simulation. Finite VLBA imaging resolution may restrict observers to seeing only the largest structures (the m = ±1 modes), while it may be possible to resolve smaller-scale structure in simulations. With the “Observing” Jet/Accretion Disk/Black Hole (JAB) simulations methodology, we may analyze disk/jet magnetohydrodynamic interactions to be exhibited by the EHT.