The discovery of new planets beyond our solar system, in particular the detection and characterization of other habitable planets similar to the Earth, is a...
Expanding our horizon: probing the architecture of planetary systems with HARPS and TESS
In order to understand the formation and evolution of small terrestrial planets not only their internal structure but also the architecture of their host system...
Exploring the diversity of exoplanet atmospheres from the ground with the ACCESS Survey
One of the most exciting possibilities enabled by transiting exoplanets is to measure their atmospheric properties through the technique of transmission...
Finding extra-solar planets in the presence of stellar jitter
The RV method is responsible for discovering the majority of planets that orbit stars other than our Sun. However, one problem with this technique is that...
Fingerprints of our Neighbors: A Spectral Library for Characterizing the Coldest Stars, Brown Dwarfs and Extrasolar Planets.
Over the past two decades, advances in infrared instrumentation have allowed us to identify a vast and previously unseen population of low-temperature stars...
First Release of PLATO Consortium Stellar Limb-darkening Coefficients
We release the first grid of stellar limb-darkening coefficients (LDCs) and intensity profiles (IPs) computed by the consortium of the PLAnetary Transits and...
Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Transmission Spectroscopy
Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up...
Gliese 486 b: una piedra de Rosetta para el estudio de los exoplanetas
Un equipo científico internacional, en el que participa el Institutito de Astrofísica de Canarias (IAC), ha medido la masa y el radio de un exoplaneta similar a...