This page lists funded projects (national funding, European funding, and cooperation projects) (co-)led by Group members, as well as missions/instruments in which we are strongly involved. Listed funded projects have a closing date no earlier than 1 Jan 2021 (for older projects, please follow this link).
Unravelling the mystery of substellar object formation
There are at least 100 billion brown dwarfs and rogue planets in our galaxy. Several theories related to processes of their formation have
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Using Ap stars as LABoratories for probing chemical transport mechanisms, with ultra-precise space-based photometry (ApLAB)
Over the last decades, asteroseismology has blossomed thanks to the ultra-precise, space-based photometric time series acquired by satellites such as CoRoT (France/ESA; 2006-2012),
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Cool Stars in the near-Infrared (CSI)
This project takes advantage of our privileged access to the Guaranteed Time Observations (GTO) data from the NIRPS (Near InfraRed Planet Searcher) spectrograph
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Star-exoplanet compositional link: Towards realistic characterisation of terrestrial planets (EXO-TERRA)
Over the last decade, noticeable advances were made in the modelling of the internal properties of terrestrial planets. It is, for instance, known
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SSA P3-SWE-XXXVII SWE Products for Southern Europe – Phase 1 (PROSE)
This project will focus on enhancing and maturing space weather assets in Southern Europe, building on the results of the preceding SSA studies
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Exploring the red side of cool stars with exoplanets
The determination of accurate and precise stellar parameters and chemical abundances of M dwarfs is of prime importance to the study of Galactic
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Stellar rotation and magnetism in the era of ultra-precise space-based photometry
Stellar brightness variations result from the contribution of different stellar phenomena at different timescales. For solar-type stars, at long timescales the brightness variations
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Space Weather Awareness Training Network (SWATNet)
SWATNet is an H2020 Marie Skłodowska-Curie Actions (MSCA) Innovative Training Network (ITN). The project brings together nine beneficiaries (including the University of Coimbra)
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A synergetic approach to the study of the Milky Way, its stars and planets using ultra-precise, space-based photometry
New insights on stellar interiors physics and evolution are being made possible by asteroseismology, the study of stars by means of their natural
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Precise characterization of exoplanets with Cheops
Cheops is the first ESA mission dedicated to the characterization of known transiting exoplanets by means of ultra-high-precision photometry of bright stars. Data
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Shedding a new light on outstanding problems in stellar physics with ultra-precise space-based photometry
The last decade has witnessed a dramatic advance in stellar physics research driven by exquisite space-based seismic data now available for thousands of
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SPIRou@CFHT
SPIRou (SPectropolarimètre InfraROUge) is a near-infrared spectropolarimeter and high-precision velocimeter for the Canada-France-Hawaii Telescope (CFHT). It is a near-infrared fiber-fed, double-pass cross-dispersed spectrograph, based
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PLATO
PLATO (PLAnetary Transits and Oscillations of stars) is an M3 ESA mission expected to launch in 2026. It is designed to find and
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Past projects
Portuguese Regional Ionosphere ModEl (PRIME)
This project aims at developing a prototype for an empirical model to forecast total electron content (TEC) variations across Portugal in response to
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Revealing the Milky Way with Gaia (MW-GAIA)
MW-GAIA will provide European leadership in understanding the Galaxy, its stars and planets, enhance the potential of the community in its scientific exploitation
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Breaking through outstanding problems in stellar evolution with ultra-precise space-based photometry (BreakStarS)
The last decade has witnessed a dramatic change in stellar astrophysics research as a result of the launch of space missions — such
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Characterizing the smallest planet hosts
The determination of accurate and precise stellar parameters and chemical abundances of M dwarfs is of prime importance to the study of Galactic
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Zoom-In ON hIgh-mass Star forMation
The theory of high-mass star formation predicts specific features, namely, the formation of near-equal binary systems, radiative Rayleigh-Taylor instabilities, and bloated photospheres. The
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