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Washington University in St. Louis News & Information > Faculty Experts at Washington University in St. Louis >

Associate professor of physics in Arts & Sciences
Expertise: gamma-rays, black holes, stars, galaxies, cosmology, solar system, astronomy, X-ray observations, VERITAS, Cherenkov telescopes, space-born X-ray telescopes, gamma-ray telescopes
Bio:
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| Krawczynski |
Professor Krawczynski works in the field of high energy astrophysics. He studies the astrophysics of supermassive black holes, which are found at the centers of galaxies. X-ray and gamma-ray observations make it possible to explore the physical conditions in the surroundings of the black holes, and to study the highly relativistic collimated plasma outflows (jets) that are produced by accretion of interstellar matter onto the black holes. Furthermore, the gamma-ray observations can be used to measure the intensity and the energy spectrum of the intergalactic infrared and optical radiation fields which absorb gamma-rays in pair-production absorption processes.
These latter measurements give unique constraints on the early history of structure and star formation in our universe. Another research topic concerns the study of high-energy particle populations that carry a significant fraction of the random energy of galaxies and galaxy clusters and influence important processes like star formation. Krawczynski's research uses the data from the ground based TeV gamma-ray telescope VERITAS and the satellite borne X-ray and gamma-ray telescopes RXTE, INTEGRAL, Suzaku, and Chandra.
WUSTL Contact Information:
Education:
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Ph.D. in Physics at University of Hamburg
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M.S. in physics at University of Hamburg

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Extremely high energy
 Pinpointing origin of gamma rays from a supermassive black hole

July 2,
2009 --
An international collaboration of 390 scientists reports the discovery of an outburst of very-high-energy gamma radiation from the giant radio galaxy Messier 87 (M 87), accompanied by a strong rise of the radio flux measured from the direct vicinity of its supermassive black hole. The combined results give first experimental evidence that particles are accelerated to extremely high energies in the immediate vicinity of a supermassive black hole and then emit the observed gamma rays. The gamma rays have energies a trillion times higher than the energy of visible light. Washington University in St. Louis physicists helped coordinate this cooperative project, the results of which appear in the July 2 Science Express, the advance online publication of the journal Science.

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Additional Background: As a member of the Very Energetic Radiation Imaging Telescope Array System (VERITAS) collaboration, Professor Krawczynski participated in the construction of a system of four Cherenkov telescopes at Mount Hopkins, Ariz. Each telescope has an optical reflector of 36 feet diameter. The telescope system detects the Cherenkov light of so-called extensive air showers that cosmic GeV/TeV photons initiate in the earth's atmosphere. Professor Krawczynski works on the astrophysical interpretation of the incoming science data and the development of control software. Furthermore, he is involved in the development of a follow-up experiment.
Professor Krawczynski works on the development of the space-borne Energetic X-ray Imaging Survey Telescope (EXIST). The mission is designed to survey the entire X-ray sky every 95 minutes. It has the potential to revolutionize our understanding of how supermassive black holes form and grow. Furthermore, it will be an ideal observatory for detecting very distant explosions (gamma-ray bursts).
In his laboratory, Professor Krawczynski fabricates and tests thick Cadmium Zinc Telluride (CZT) semiconductor detectors for space-borne X-ray and gamma-ray telescopes. The detectors achieve excellent spatial and energy resolutions without cryogenic cooling. The group specializes on the fabrication of pixelated detectors using photolithographic techniques and pioneered several novelties such as "electrically isolated'" steering grids that steer electrons to the detector pixels while suppressing grid-pixel currents, which deteriorate the detectors' energy resolutions.
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