PASTIS

Planet Analysis and Small Transit Investigation Software

Coordinatore	CENTRO DE INVESTIGACAO EM ASTRONOMIA E ASTROFISICA DA UNIVERSIDADE DO PORTO    more  Organization address address: Rua das Estrelas city: Porto postcode: 4150-762 contact info Titolo: Mrs. Nome: Elsa Cognome: Silva Email: send email Telefono: +351 226089830 Fax: +351 226089831
Nazionalità Coordinatore	Portugal [PT]
Totale costo	153˙330 €
EC contributo	153˙330 €
Programma	FP7-PEOPLE Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	FP7-PEOPLE-2013-IEF
Funding Scheme	MC-IEF
Anno di inizio	2014
Periodo (anno-mese-giorno)	2014-10-01   -   2016-09-30

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	CENTRO DE INVESTIGACAO EM ASTRONOMIA E ASTROFISICA DA UNIVERSIDADE DO PORTO  Organization address address: Rua das Estrelas city: Porto postcode: 4150-762 contact info Titolo: Mrs. Nome: Elsa Cognome: Silva Email: send email Telefono: +351 226089830 Fax: +351 226089831	PT (Porto)	coordinator	153˙330.00

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 Obiettivo del progetto (Objective)

'Detection and characterization of extrasolar low-mass planets are currently limited by several astrophysical and instrumental effects. New exoplanet-hunter instruments, with improved capabilities, are foreseen at the horizon 2016 - 2017. To find other Earths, new state-of-the-art instruments must be followed by the state-of-the-art of data analysis software that takes into account for the astrophysical limitations. Currently, the main astrophysical limitations to the detection and the precise characterization of exoplanets are the precise characterization of the host star and the existence of false-positive scenarios (such as diluted binaries or stellar activity which are able to mimic extrasolar planets. The objective of this proposal is double. First, implement into the PASTIS software (a state-of-the-art of data-analysis software, co-developed by the candidate) tools to both characterize the planet-host star and to model stellar jitter. This will be done with the help of world-leading experts present at the host institution. The second objective is to validate new small and low-mass planets among the CoRoT, Kepler and HARPS data, using the improved PASTIS software. These developments and detections will be a milestone for the detection capabilities and analysis of data currently collected at the host institution and for the search of exo-Earths with future facilities, in which Europe always played a pioneer role.'