The advantage of large optical telescopes from the ground for high-contrast direct imaging relies on achieving exquisite control of the incident optical...

Table 2 contains the Atomic parameters and measured solar equivalent widths for FeII and Fe I lines. (1 data file).

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 is the proposed ultra-stable optical high-resolution spectrograph for the E-ELT, which will use novel Laser Comb calibration techniques and an innovative...

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...

A number of outstanding scientific problems require a high resolution, visual spectrograph at the E-ELT. Measuring the dynamics of the universe, finding earth...

Accretion onto a supermassive black hole (BH) is the most viable explanation for the huge emitted luminosity in active galaxies. Nowadays a wealth of...

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...

A sample of spiral galaxies is examined, applying moments analysis to their broad-band azimuthal profiles, in order to search for evidence of coherent large...