Slide 1 what good are low frequencies? HI, neutral hydrogen, H 0, atomic hydrogen high redshifts and early times…. USS, GPS, … “enabling technologies” …multi-beaming,…

Hirotaka Ito 　YITP, Kyoto University　　　 Emissions from Shells Associated with Dying Radio Sources ＠Workshop on East-Asian Collaboration for the SKA　2011 12/2…

what good are low frequencies? HI, neutral hydrogen, H0, atomic hydrogen high redshifts and early timesâ¦. USS, GPS, ⦠âenabling technologiesâ â¦multi-beaming, all-sky…

Titel models: what drives the correlations ?? - high Eddington-scaled accretion rate and/or - low BH mass - density effect - orientation - young age - different host galaxies…

On the role of density and Eddington ratio in the correlation space of NLS1 galaxies May 14, 2013 Dawei Xu National Astronomical Observatories, Beijing In coll. With S. Komossa,…

Radio Galaxies Part 5 Unified schemes are all AGNs really different? What is the life of a radio galaxy? - do we know which one are the newly-born radiogalaxies? - what do…