Sheperd S. Doeleman

Sheperd "Shep" S. Doeleman (born 1967) is an American astrophysicist. His research focuses on super massive black holes with sufficient resolution to directly observe the event horizon. He is a senior research fellow at the Harvard–Smithsonian Center for Astrophysics and the director of the Event Horizon Telescope project.[1] He led the international team of researchers that produced the first directly observed image of a black hole.[2][3]

Sheperd S. Doeleman
Born
Sheperd Nackeman

1967
Scientific career
FieldsAstrophysics
InstitutionsMassachusetts Institute of Technology, Max Planck Institute for Radio Astronomy, Harvard–Smithsonian Center for Astrophysics
ThesisImaging Active Galactic Nuclei with 3mm-VLBI (1995)
Doctoral advisorsAlan E.E. Rogers and Bernard F. Burke

Background

He was born in Wilsele in Belgium to American parents. The family returned to the United States few months later, and he grew up in Portland, Oregon. He was later adopted by his stepfather Nelson Doeleman.[4]

Career and research

He earned a B.A. at Reed College in 1986 and then spent a year in Antarctica working on multiple space-science experiments at McMurdo Station. He then went on to earn a PhD in astrophysics at the Massachusetts Institute of Technology (MIT) in 1995; his dissertation was titled Imaging Active Galactic Nuclei with 3mm-VLBI. He has worked at the Max Planck Institute for Radio Astronomy in Bonn and returned to MIT in 1995, where he later became assistant director of the Haystack Observatory.[5][6]

His research has focused in particular on problems that require ultra-high resolving power. He is known for heading the group of over 200 researchers at research institutions in several countries that produced the first simulated image of a black hole.[3]

Significant papers

  • Doeleman S.S., et al. (2008). Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre. Nature 455: 78–80.
  • Doeleman S.S., et al. (2012). Jet-Launching Structure Resolved Near the Supermassive Black Hole in M87. Science 338: 355–358.
  • Doeleman S.S., et al. (2009). Detecting Flaring Structures in Sagittarius A* with High-Frequency VLBI. Astrophys.J 695: 59-74.

Awards

gollark: Anyway, if someone wants I can probably make an adapter to call some other process so you can write JS or whatever. It will just be slow and unpleasant.
gollark: That was needless and unhelpful.
gollark: ...
gollark: Besides, scheme would allow coolness like prisoner's-dilemma-with-visible-source at some point.
gollark: Or heavpoot's lua-based one, even.

References

  1. "Sheperd Doeleman". bhi.fas.harvard.edu.
  2. "Harvard scientists shed light on importance of black hole image". 10 April 2019.
  3. Ghosh, Pallab (10 April 2019). "First ever black hole image released". BBC.
  4. Seth Fletcher: Einstein's Shadow: A Black Hole, a Band of Astronomers, and the Quest to See the Unseeable (part 1, chapter 3). HarperCollins, 2018, ISBN 978-0-06-231202-0
  5. "Sheperd S. Doeleman". John Simon Guggenheim Foundation.
  6. "Sheperd S. Doeleman".
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.