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The Stellar Characterisation working group team
The Stellar Characterisation working group team
The stellar characterisation WG is composed by scientists specialised in different field of the stellar characterisation. The team is mostly composed by European members, with collaborations from NASA and JPL (US).
The working group is divided in different sub-working groups, each one responsible for determining different sets of stellar parameters.
The Team works closely in synergy within other WG within the Ariel Consortium and with other consortia within and outside Europe.
The WG scientific coordinator
The WG scientific coordinator
Camilla Danielski
(University of Valencia, Valencia, Spain)
Camilla Danielski
(University of Valencia, Valencia, Spain)
Camilla coordinates the activities between the various sub-WGs and all the synergies within and beyond the Ariel consortium.
The sub-WGs coordinators
The sub-WGs coordinators
Observations:
Monica Rainer (INAF - Osservatorio Astronomico di Brera, Brera, Italy )
Kris Helminiak (N. Copernicus Astronomical Center, Toruń, Poland)
Atmospheric parameters: Laura Magrini (INAF - Osservatorio Astrofisico di Arcetri, Florence, Italy)
Elemental abundances: Elisa Delgado Mena (Centro de Astrobiología (CAB), CSIC-INTA, Madrid, Spain)
Age, Mass, Radius:
Tiago Campante (Universidade do Porto, Oporto, Portugal)
Andy Moya (University of Valencia, Valencia, Spain)
Activity indexes: Serena Benatti (INAF - Osservatorio Astronomico di Palermo, Palermo, Italy)
Multi-bandpass images of the Sun. (Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.
The synergies within the Ariel consortium
The synergies within the Ariel consortium
The working group closely works with other working groups in the Ariel consortium. In particular our synergies are with:
The planetary formation WG: Diego Turrini (INAF - Osservatorio Astronomico di Torino, Turin, Italy).
The stellar activity WG:
Giusi Micela (INAF - Osservatorio Astronomico di Palermo, Palermo, Italy).
Bart Vandenbussche (KU Leuven, Leuven Belgium).
Ignasi Ribas (IEEC– CSIC, Spain).
The planetary mass WG:
Giusi Micela (INAF - Osservatorio Astronomico di Palermo, Palermo, Italy).
Lars Buchave (DTU Space, Technical University of Denmark)
The Simulations WG: Billy Edwards (SRON, Netherlands Institute for Space Research).
ExoClock: Angelos Tsiaras (Aristotle University of Thessaloniki, Thessaloniki, Greece).
Anastasia Kokori (University College London, London, UK).
The star-planet interaction & activity diagnostics sub-WG: Sudeshna Boro Saikia (Department of Astrophysics, Vienna, Austria).
Stellar surface modelling sub-WG: Stefano Bellotti (Leiden Observatory, Leiden University, Leiden, The Netherlands).
The synergies in Europe
The synergies in Europe
The SPICA consortium - Roxanne Ligi (Observatoire de la cote d'Azure, Nice, France)
Denis Mourard (Observatoire de la cote d'Azure, Nice, France)
Andrea Chiavassa (Observatoire de la cote d'Azure, Nice, France)
The CARMENES consortium, in particular the Stellar Parameters WP.
Observatori del Montsec - Gemma Domènech Rams
The synergies outside Europe
The synergies outside Europe
David W. Latham (Harvard CFA, Cambridge, MA, USA)
David Ciardi (Caltech/IPAC - NASA Exoplanet Science Institute)
George Helou (Caltech/IPAC)
Douglas Hudgins (NASA HQ)
Norio Narita (University of Tokyo, Tokyo, Japan)
The Kepler Orrery: 1,791 candidate planets discovered transiting 709 different stars by NASA's Kepler space telescope showing the variety of stars hosting exoplanets (Credit: NASA, based on catalog of Lissauer et al. 2023)
Would you like to be part of the team ?
Would you like to be part of the team ?
Contact us by email at scwgariel AT gmail.com
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