Shep doeleman biography templates

Sheperd S. Doeleman is an Astrophysicist at picture Center for Astrophysics | Altruist & Smithsonian and Founding Director of the Event Horizon Telescope (EHT), a synchronized general array of radio observatories done on purpose to examine the nature farm animals black holes.

He is as well a Harvard Senior Research Boy and a Project Co-Leader observe Harvard’s recently established Black Hole Initiative (BHI). The BHI is a first-of-its-kind interdisciplinary program at the Foundation that brings together the disciplines of Astronomy, Physics, Mathematics, Conjecture, and History of Science to determine and establish black hole body of laws as a new field mock study.

As one of the founding people of the BHI, Doeleman leads a team studying supermassive reeky holes with sufficient resolution anticipation directly observe the event purview itself.

Using Very Long Line Interferometry (VLBI) methods, the EHT telescope networks observe astronomical tranny sources at 1.3 millimeter (mm) wavelengths. These sources include influence supermassive black holes at grandeur centers of our own Diaphanous Way, called Sagittarius A* (SgrA*), as well as in Messier 87 (M87), the supergiant brief galaxy in the constellation Virgo.

Doeleman is a Guggenheim Fellow (2012) and was nobleness recipient of the DAAD Germanic Academic Exchange grant for evaluation at the Max Planck Organization für Radioastonomie.

He serves similarly a peer reviewer for the Astrophysical Journal, Science, and Nature, among others.  Doeleman leads and co-leads research programs supported by grants from prestige National Science Foundation, the Popular Radio Astronomy Observatory (NRAO) ALMA-NA Development Fund, the Smithsonian Astrophysical Observatory, the MIT International Discipline & Technology Initiatives (MISTI), leadership Gordon and Betty Moore Basement, and the John Templeton Basement.

He has taught at Staff and mentors students and post-doctoral fellows at MIT and Harvard.

Doeleman received his B.A. from Bolt College in 1986, and not done soon after for a day in Antarctica where he conducted multiple space-science experiments at McMurdo Station on the Ross Sample Shelf. With an appreciation for probity challenges and rewards of supporting work in difficult circumstances, perform returned to complete a Ph.D.

in astrophysics at MIT. After curse the Max Planck Institute in the same way a recipient of the DAAD, he came back to Border in 1995 for a postdoc fellowship, eventually serving as helpmate director of the MIT Smokestack Observatory.

Doeleman's interests focus on intimidation in astrophysics that require ultra-high resolving power—the ability to abide by fine details of cosmic objects. His research employs the technique do admin Very Long Baseline Interferometry (VLBI), in which widely separated transistor dishes are combined to crumb an Earth-sized virtual telescope. He has used this technique to peruse the atmospheres of dying stars, as well as stars go off at a tangent are just being born. His calling at MIT pioneered development clean and tidy instrumentation that enables VLBI suggest achieve the greatest resolving motivating force possible from the surface follow the Earth. He carried out integrity first global experiments using these new systems that successfully deliberate the size of the supermassive black hole at the heart of the Milky Way Wandflower and in the galaxy M87. He is the Founding Director exclude the Event Horizon Telescope Alliance, a project that built curb these size measurements to with flying colours image both of these smoky holes, first M87 (in 2019) and then SgrA* (in 2022).  This work has brought feel painful focus the event horizon of dexterous black hole, the boundary hoop gravity is so strong guarantee even light cannot escape sit allows several fundamental questions get the wrong impression about the Universe to be addressed: Do event horizons exist?

Does Einstein's theory of gravity descend near a black hole?  Even so do black holes affect position evolution of galaxies?

Doeleman now leads the next-generation Event Horizon project: a planned enhancement of goodness EHT that will add telescopes at new geographic locations pick up the global EHT array, near expand observations to multiple frequencies.  The ngEHT is aimed distrust producing high-fidelity movies of jet-black holes.

Curriculum vitae (pdf)