Co-Evolution of Supermassive Black Holes and Their Host Galaxies
We study the evolution of the MBH/Mhost relation up to z = 3 for a sample of 96 quasars with known host galaxy luminosities. Black hole masses are estimated...
CODEX is the proposed ultra-stable optical high-resolution spectrograph for the E-ELT, which will use novel Laser Comb calibration techniques and an innovative...
Many talks in this conference have shown the power of high resolution spectroscopy, coupled to high precision. A new spectrograph, fed by an Extremely Large...
CODEX: An Ultra-stable High Resolution Spectrograph for the E-ELT
CODEX is the proposed optical high resolution spectrograph for the E-ELT. Designed to make the most of the unique light-gathering power of the E-ELT and to...
CODEX: the high-resolution visual spectrograph for the E-ELT
A number of outstanding scientific problems require a high resolution, visual spectrograph at the E-ELT. Measuring the dynamics of the universe, finding earth...
Coevolution of supermassive black holes and their host galaxies
Accretion onto a supermassive black hole (BH) is the most viable explanation for the huge emitted luminosity in active galaxies. Nowadays a wealth of...
Coevolution of Supermassive Black Holes and Their Host Galaxies
Accretion onto a black hole (BH) is the most viable explanation for the huge emitted power in active galaxies. A wealth of observations have shown the presence...