We are developing and will commission a space debris and satellite imaging system in New Zealand to improve image resolution of Earth orbiting objects. Our...
Adaptive Optics research at the Institute of Optics and Electronics, Chinese Academy of Sciences
The research and development on adaptive optics in China began in 1979. Prof. Jiang from the Institute of Optics and Electronics, Chinese Academy of Sciences...
Luminous Infrared Galaxies (LIR=10^11-10^12Lsun) have star formation rates in the range of ~20-200Msun/yr. In the local Universe ~50% LIRGs show AGN or AGN/SB...
AGN feedback from Mpc to pc scale: radio-mode, quasar-mode and backflows
Mechanical feedback by jets from Active Galactic Nucei (AGN) is a key process in galaxies and galaxy clusters: the energy input from the jets (in literature...
Over the past decade there has been a growing body of evidence for a closely regulated balance of heating and cooling of the intracluster medium in the cores of...
AGN winds, feedback and the baryon cycle in the galaxy ecosystem
Why did galaxies stop forming stars? Why do black holes in galactic nuclei have masses proportional to bulge masses? What are the physical mechanisms leading...
SOFIA, short for Stratospheric Observatory for Infrared Astronomy, is a 2.7m telescope flying on a Boeing 747SP at altitudes of 12-14km, to detect and study mid...
Airglow in the atmospheres of the terrestrial planets
There is a multitude of photochemical processes occurring in a planet's atmosphere. Some of these processes occur with an excess of energy and lead to products...