Virtual Observatory Science and the ARCHES project
The Virtual Observatory (VO) is an international astronomical community-based initiative. It aims at providing easy and efficient access and analysis of the...
VO Tools: an overview on Virtual Observatory tools
The Virtual Observatory is an international initiative on standardizing astronomical data and protocols, as well as the development of scientific tools...
Observational studies show that voids are prominent features of the large scale structure of the present day Universe. Even though their emerging from the...
Warps of disk galaxies are ubiquitous. In almost every disk galaxy a bending of the disk occurs where the stars fade away and hence where the dark matter halo...
WEAVE: The next generation wide-field spectroscopy facility for the WHT
I will describe the major scientific motivation and outline design concept for a new 2 degree field, 1000 fibre multi-object spectroscopy facility for the WHT...
What do we learn from radar observations of asteroids and comets?
Radar observation of near-Earth asteroids (NEAs) reveal the size, shape, spin characteristics of the population of small bodies near the Earth. Although...
What is the Milky Way outer halo made of? High resolution spectroscopy of distant red giants
In a framework where galaxies form hierarchically, extended stellar haloes are predicted to be an ubiquitous feature around Milky Way-like galaxies and to...
What is the role of the environment in shaping early-type galaxy sizes? Did it changed in the last 10 Gyr?
Understanding galaxy evolution requires understanding the impact of cosmic time, environment, mass, and halo growth at least, because likely a combination of...
Recent advances in 3D model atmospheres have led to a significant downward revision in photospheric heavy element abundance estimates for the Sun, especially...