We find that Centaurus A's source structure resembles the jet in Messier 87 on ${\sim}500r_g$ scales remarkably well.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena
We investigate the capability of an advanced EHT concept, including an orbiting space antenna, to image and distinguish different spacetimes around Sgr A*.
High Energy Astrophysical Phenomena Astrophysics of Galaxies General Relativity and Quantum Cosmology
The detailed analysis of our simulations shows that the structure and properties of the observed relativistic jets in NGC 1052 can be reconstructed by a slightly over-pressured jet ($d_k\sim1. 5$) embedded in a decreasing pressure ambient medium
High Energy Astrophysical Phenomena Astrophysics of Galaxies
These studies are important when proposing observations of new sources, in the characterization of the capabilities of new or upgraded instruments, and when verifying model-based theoretical predictions in a comparison with observational data.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
We hope that such a public tool can be useful in the context of the recent and near-future GRAVITY and EHT results.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
We perform quantitative measurements of relevant polarimetric properties of the compact emission and find evidence for the temporal evolution of the polarized source structure over one week of EHT observations.
High Energy Astrophysical Phenomena Astrophysics of Galaxies
Polarimetric MEM is thus an attractive choice for image reconstruction with the
Instrumentation and Methods for Astrophysics Astrophysics of Galaxies
We present a scattering mitigation framework for radio imaging with very long baseline interferometry (VLBI) that partially overcomes this limitation.
Instrumentation and Methods for Astrophysics Astrophysics of Galaxies
Most recently, the Event Horizon Telescope (EHT) has extended VLBI to short millimeter wavelengths with a goal of achieving angular resolution sufficient for imaging the event horizons of nearby supermassive black holes.
By linking widely separated radio dishes, the technique of very long baseline interferometry (VLBI) can greatly enhance angular resolution in radio astronomy.
Instrumentation and Methods for Astrophysics