http://dfe.iaa.csic.es/persia/wiki/ 2026-04-10T05:13:11+00:00 http://dfe.iaa.csic.es/persia/wiki/ http://dfe.iaa.csic.es/persia/wiki/lib/tpl/dokuwiki/images/favicon.ico text/html 2015-03-29T19:15:08+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp1&rev=1427656508&do=diff WP1. Coordination & Management Responsible Other ParticipantsUGR IRAP Management of the project including elaboration of reports, organisation of periodic meetings, workshops, and responsible of the website of the project Taks * Organisation of periodic meetings of the project board text/html 2015-03-27T19:54:31+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp2&rev=1427486071&do=diff Exploitation of the pulsating frequency content in rapidly rotating stars Responsible Antonio García Hernández (AGH) Work Package number: WP2 Work Package title: Exploitation of the pulsating frequency content in rapidly rotating pulsating stars text/html 2015-03-30T09:20:31+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp3&rev=1427707231&do=diff WP3. 2D structure modelling of rotating stars deformed by the centrifugal force Responsible Jerôme Ballot Compute realistic models of rotating stars deformed by the centrifugal force and provide a grid of models with seismic indices. Tasks * Compute static 2D models that fit constrains on classical stellar global parameters and seismic indices text/html 2015-03-23T10:56:32+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp4&rev=1427108192&do=diff WP4. Modelling the oscillation spectra of rotating stars Responsible Marc-Antoine Dupret possible tasks : 1. Non adiabatic oscillations of rapidly rotating stars : Daniel Reese has just developped a non-adiabatic version of the TOP code. This offers the unique possibility to study the effect of rapid rotation on mode excitation. First results have been shown Reese (2015 arXiv:1502.01696) but a lot of work is needed to cover the different pulsating stars of the upper HR diagram. This task requ… text/html 2015-03-27T15:51:05+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp5&rev=1427471465&do=diff WP5. Virtual Observatory archives and tools. Responsible Enrique Solano (ES) Work Package number: WP5 Work Package title: Virtual Observatory archives and tools Lead partner: INTA Participants and person/months per participant: * INTA: 48 * text/html 2015-03-30T13:43:34+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp6&rev=1427723014&do=diff WP6. Spectroscopic analysis Responsible: INAF Ennio Poretti The space mission CoRoT and Kepler observed hundreds of A-F type stars locate inside the instability strip. Spectroscopic campaigns in the framework of three ESO Large Programmes (LPs) were performed and some papers were published (see below). text/html 2015-04-03T18:08:53+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp7&rev=1428084533&do=diff WP7. Lightcurve analysis Responsible Rafael Garrido General objective Analysis of photometric lightcurves - development of open source tools for data processing Specific objectives * Correct gap fillings in time series * Selfconsistent analysis of time measurement text/html 2015-03-26T15:47:34+00:00 Anonymous (anonymous@undisclosed.example.com) http://dfe.iaa.csic.es/persia/wiki/doku.php?id=work:wp8&rev=1427384854&do=diff WP8. Outreach, dissemination & sustainability Responsible Other Participants INTA ALL Ensure that scientific and technological communities related to the project know about the work of PERSIA. Provide generic outreach for the use and understanding for expert and non-expert potential users of the tools and data generated by the project. Define the strategy for long-term support and sustainability of the tools and data generated within the PERSIA project.