How to image black holes? VLBI and radio interferometry explained!
In this video, I explain the Very Long Baseline Interferometry(VLBI) technique which is used by the Event Horizon Telescope (EHT) to image the shadow of the black hole M87* and SAG A*. I also explain the basics of radio astronomy and talk about telescopes to help understand the topic well. In July 2022 my research group and I visited #MIT's Haystack Observatory to discuss our balloon-borne project. Had this fantastic experience of not only meeting some of the most amazing and smart people but also learning a lot about astronomy, instrumentation, and science in general! Let me know if you have any doubts about whatever you see. See you guys soon! Timestamps : 0:00 Intro 1:59 EM Spectrum 4:37 What are radio telescope 6:30 Imaging a Black Hole: VLBI 13:44 Outro

How did they actually take this picture? (Very Long Baseline Interferometry)

Understanding Radio Telescopes: Dr John Morgan

The new BLACK HOLE image explained by an ASTROPHYSICIST | Your questions answered

Pushing Simulations to the LIMIT to Find Order in Chaos

Astrophysicists Discuss the Fermi Paradox

Basic Radio Interferometry I

Sagittarius A* Might Not Be a Black Hole

Introduction to Radio Astronomy (English)

Computational Imaging for VLBI Image Reconstruction

Brian Cox: Why even Einstein doubted the existence of black holes

Is the Soul Real? Neuroscience’s Surprising Answer

How Does Burj Khalifa Get Water to the 163rd Floor

The Absurd Search For Dark Matter

Beyond the Visible: The Story of the Very Large Array

VLBI Data Series 3: Imaging Techniques

The Mathematical Problem with Music, and How to Solve It

What Is a Photon Actually Made Of… And Why Does It Never Stand Still?

Why This Black Hole Photo is Different?

Turning Waves Into Particles

