Technique - (3) Multi-wavelength VLBI imaging of black hole accretion flows (Event Horizon Telescope)

Type: Experimental

Description:

Department(s)/lab(s): Astronomy | Event Horizon Telescope Group (Doeleman) @ Harvard
Summary:

Doeleman founded and directs the Event Horizon Telescope, assembling a global mm-wavelength VLBI network to image the immediate environments of supermassive black holes at horizon-scale resolution — an astronomy pivot whose entire scientific case rests on pushing angular resolution to its fundamental (diffraction/baseline) limit via a globally distributed, highly complex sensor array.

Department(s)/lab(s): Astronomy | Johnson VLBI Group @ Harvard
Summary:

Johnson studies neutron stars and black holes via extreme-resolution VLBI imaging, including direct observation of magnetic fields and orbital dynamics near black-hole event horizons as part of the Event Horizon Telescope collaboration, pushing spatial resolution to the horizon scale.

Department(s)/lab(s): Institute of Astronomy / Kavli Institute for Cosmology | Markoff Group @ Cambridge
Summary:

Markoff studies the extreme physics of accretion and jet formation around black holes of all scales, combining multi-wavelength observations with computational simulations; she is a founding member of the Event Horizon Telescope collaboration that produced the first black hole images, and co-leads a new EHT station in Namibia.