A Technical Overview of the Thirty Meter Telescope (TMT)
This presentation will describe the subsystems of the Thirty Meter Telescope Observatory (TMT), with a focus on the technical aspects. In general, large...
A tool for restoring the starry sky at Teide Observatory
Increasing light pollution is a threat to the research capacity of astronomical observatories. The case of the Teide observatory is not an exception, despite...
Active galactic nuclei synapses: X-ray versus optical classifications using artificial neural networks
The active galactic nuclei is conformed by a number of classes. Optically they are defined using diagnostics based on optical emission lines. At X-rays they are...
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...