Tony Readhead

Observational Cosmology and Active Galaxies

My main areas of interest are observational cosmology, especially the cosmic microwave background radiation, and active galaxies, with special emphasis on the central engines that drive them and the formation of relativistic jets. In carrying out research in both these areas I am particularly interested in developing state-of-the-art instrumentation.

Over the last ten years I led the Cosmic Background Imager (CBI) project in Chile, and this has now been superseded by the QU Imaging ExperimenT (QUIET) project at the same site. In Phase I, we demonstrated the feasibility of using Monolithic Millimeterwave Integrated Circuits (MMICs) for making very sensitive observations of the cosmic microwave background, and we are now embarking on QUIET Phase II, with which we hope to detect the large-scale B-mode polarization radiation caused by gravitational waves interacting with the CMB. The detection of this signal would prove that the universe did go through an inflationary phase, reveal the energy scale of inflation, possibly pushing the clock back to 10-35 s after the Big Bang. Our new radio laboratory in Cahill is working closely with JPL and Northrop Grumman Corporation to improve the sensitivity of the MMIC amplifiers.

The other side of my research involves the engines that drive the activity in active galaxies. Our group, in collaboration with several others, developed the Very Long Baseline Interferometry (VLBI) imaging techniques that are in wide use today, and we are using VLBI to study a carefully selected sample of blazars that are also being observed with Fermi-GST, and in addition we are observing the TeV sources being monitored by VERITAS. Our program of 15 GHz monitoring of the light curves of ~1200 blazars on the Owens Valley Radio Observatory (OVRO) 40m Telescope twice a week is the most comprehensive variability study of active galaxies thus far and is providing key information on these objects.

I work very closely with my students and postdocs, and they get a lot of experience on different instruments -- radio, submm, IR, optical, X-ray, gamma-ray -- often helping to build new instruments. After leaving my group we always keep in touch and very often continue collaborating for many years.

[Image credits: A. Readhead; S. Radford/Caltech]