Dr. Joseph Hennawi

Profile

Academic positionAssociate Professor, Senior Lecturer, Reader
Research fieldsAstronomy,Astrophysics
Keywordsthe intergalactic medium, active galactic nuclei, quasar absorption lines, cosmic reionization

Current contact address

CountryUnited States of America
CityBerkeley
InstitutionUniversity of California, Berkeley
InstituteAstronomy Department

Host during sponsorship

Prof. Dr. Hans-Walter RixMax-Planck-Institut für Astronomie, Heidelberg
Start of initial sponsorship01/07/2010

Programme(s)

2010Sofja Kovalevskaja Award Programme

Nominator's project description

The most barren regions of the Universe are the vast expanses between the galaxies, known as the intergalactic medium. Averaging just one lonely atom per cubic meter, this primordial gas left over from the Big Bang encodes fundamental information about our Universe’s history. Intergalactic atoms are observable only indirectly, via their selective absorption of light traveling to Earth from distant, hyper-luminous galaxies known as quasars. Joseph Hennawi pioneered a method for finding pairs of quasars, right next to each other on the sky. He showed how these extremely rare configurations can be used to make unprecedented measurements of the small-scale structure and physical properties of intergalactic gas. Hennawi observes quasar pairs using the largest telescopes in the world; by comparing his data to supercomputer simulations of cosmic evolution, he will resolve key questions about the evolution of the Universe and shed light on how galaxies, and ultimately stars and planets, formed.