The Event Horizon Telescope (EHT) is a global millimeter very-long-baseline interferometry (VLBI) array designed to image supermassive black holes at event-horizon scales. The collaboration released the first image of the black hole in M87 in 2019 and the first image of Sagittarius A*, the black hole at the center of the Milky Way, in 2022 [EHT Collaboration et al. 2019, 2022]. This project reflects Junhan's earlier work and remains an important foundation for the lab's broader interests in radio instrumentation.
A major component of this work was the development of a dedicated VLBI receiving system for the South Pole Telescope (SPT), a 10-meter millimeter telescope at the South Pole that significantly extends the EHT's north–south baselines. To enable VLBI observations with the SPT, Junhan developed the dual-frequency receiver and coherent signal chain, carrying the system from design and integration to lab characterization, on-sky testing, and software development.
Related Publications
First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way [ADS] [arXiv]
The Event Horizon Telescope Collaboration et al., including Kim, J., 2022, ApJL, 930, L12
Event Horizon Telescope Observations of the Jet Launching and Collimation in Centaurus A [ADS] [arXiv]
Janssen, M. et al., including Kim, J., 2021, Nature Astronomy, 5, 1017
The Event Horizon Telescope Collaboration et al., including Kim, J., 2019, ApJL, 875, L2
Kim, J., Marrone, D. P., et al., 2018, Proceedings of SPIE, 10708, 107082S
Kim, J., Marrone, D. P., et al., 2018, ApJ, 861, 129
Kim, J. & Marrone, D. P., 2018, Proceedings of the 29th International Symposium on Space Terahertz Technology, 159-163