Area of research
Astronomy and Astrophysics · Nuclear and High Energy Physics
Research interest
Research interests include Physics, Astrophysics, Astronomy, Supermassive black hole, Sagittarius A*, and Galactic Center.
The persistent shadow of the supermassive black hole of M87
A multifrequency study of sub-parsec jets with the Event Horizon Telescope
Horizon-scale variability of M87* from 2017–2021 EHT observations
First Sagittarius A* Event Horizon Telescope Results. VII. Polarization of the Ring
First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring
The persistent shadow of the supermassive black hole of M 87
Broadband multi-wavelength properties of M87 during the 2018 EHT campaign including a very high energy flaring episode
Ordered magnetic fields around the 3C 84 central black hole
First Very Long Baseline Interferometry Detections at 870 μm
The putative center in NGC 1052
First M87 Event Horizon Telescope Results. IX. Detection of Near-horizon Circular Polarization
The Event Horizon Telescope Image of the Quasar NRAO 530
Comparison of Polarized Radiative Transfer Codes Used by the EHT Collaboration
Rotation in Event Horizon Telescope Movies
A Search for Pulsars around Sgr A* in the First Event Horizon Telescope Data Set
Polarimetric Geometric Modeling for mm-VLBI Observations of Black Holes
First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
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. 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. IV. Variability, Morphology, and Black Hole Mass
Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign
\nPATOKA: Simulating Electromagnetic Observables of Black Hole Accretion
Resolving the Inner Parsec of the Blazar J1924–2914 with the Event Horizon Telescope
A Universal Power-law Prescription for Variability from Synthetic Images of Black Hole Accretion Flows
Characterizing and Mitigating Intraday Variability: Reconstructing Source Structure in Accreting Black Holes with mm-VLBI