Shortly after the discovery of the first extra-solar planet, many studies showed that stars hosting giant planets have significant metallicity excess when...
Planetary Atmospheres 2: Radiative Transfer, Composition, and Clouds
Series: XXVIII Canary Islands Winter School of Astrophysics: Solar System Exploration Topic: Planetary Atmospheres. Lecture 2: Radiative transfer, composition...
Planning the WHT future: the WEAVE wide-field massive-multiplex spectrograph
The vision for the use of the WHT in the coming decade is taking shape. A key element is the construction and deployment of WEAVE, a wide-field massive...
PLATO: The ESA Cosmic Vision planetray system characterizer
I present a general overview of the PLAnetary Transits and Oscillations of stars (PLATO) space mission. PLATO was approved by ESA’s Science Programme Committee...
Current scientific cosmology hosts a plurality of scenarios that articulate in different ways the precision astronomy's observations. However, this palette of...
Population of red supergiants in dwarf irregular galaxies
The identification and investigation of red supergiants (RSGs) in the Local Group and beyond are extremely important for understanding massive star evolution...
We will start by recalling the effects of rotation on stellar evolution and briefly explain its implementation in a stellar evolution code. We will present a...
Possible photometric signatures of moderately advanced civilizations: The Clarke exobelt
This paper puts forward a possible new indicator for the presence of moderately advanced civilizations on transiting exoplanets. The idea is to examine the...
Precipitable water vapour at the Roque de los Muchachos Observatory from GPS measurements
There are many parameters accounting for the quality of an astronomical site, namely seeing, cloud cover, ground winds, high-altitude winds, etc. The water...