Name: PLATO Input Catalogue (PIC) Workshop (I)
Start: 2019-09-24T14:00:00+02:00
End: 2019-09-26T13:00:00+02:00
Location: Sala Consiliare, Provincia di Padova

Monday 23 September 2019
Tuesday 24 September 2019
14:00
14:00 - 14:10
Contributions

14:00 Welcome and Workshop purposes - Giampaolo Piotto
14:10
14:10 - 15:55
Contributions

14:10 PLATO Mission status update - Juan Cabrera

14:25 PLATO Mission science goals - Don Pollacco

14:40 The PIC in ESA Science Management Plan context - Ana Heras

14:50 PIC: general properties - Giampaolo Piotto

15:05 Previous experiences on COROT (and Kepler/K2) - Magali Deleuil (LAM)

15:25 TESS experience with the TESS Input Catalogue - Keivan G. Stassun
15:55 Coffee break
Coffee break
15:55 - 16:25
16:25
16:25 - 18:20
Contributions

16:25 P1, P2, and P5 samples: target selection criteria - Marco Montalto

16:50 The cool stars sample (P4) - Loredana Prisinzano

17:05 PIC target prioritization - Alessandro Sozzetti

17:20 Astrophysical contaminants - Bray John

17:35 Scientific validation of the PIC - Vardan Adibekyan

17:50 Discussion
Wednesday 25 September 2019
09:10
09:10 - 11:00
Contributions

09:10 Exoplanet hosts and the PIC - Don Pollacco

09:25 Multiplicity of planet hosts - Silvano Desidera

09:40 False positives: what can be done in the PIC - Alexandre Santerne

09:55 Circumbinary planets: implications for the PIC - Hans Deeg

10:10 Activity and activity cycles of PLATO target stars: PIC implications - Nuccio Lanza

10:30 Simulation of end of mission Gaia catalogue in PLATO fields - Josep Manel Carrasco

10:45 Discussion
11:00 Coffee break
Coffee break
11:00 - 11:25
11:25
11:25 - 12:35
Contributions

11:25 Stellar Science and PIC - Marie-Jo Goupil

11:40 Benchmark eclipsing binaries in the PLATO long-stare fields - Pierre Maxted

11:55 Preparatory data needed for the non-seismic characterisation of the PLATO targets - Thierry Morel

12:10 Asteroseismology model calibration - Andrea Miglio

12:25 Discussion
12:35 Lunch break
Lunch break
12:35 - 13:35
13:35
13:35 - 14:35
Contributions

13:35 Introduction to the PLATO-CS - Conny Aerts

13:45 Complementary Science and PLATOSim/TESS/Gaia/Sloan links - Andrew Tkachenko

14:00 Galactic Archaeology with asteroseismology: lessons learned with CoRoT, Kepler, K2, and TESS - Cristina Chiappini

14:15 Interior Rotation from Red Giants - Charlotte Gehan

14:25 Interior Rotation and Ages of F stars - Timothy Van Reeth
14:35
14:35 - 16:10
Contributions

14:35 The inputs to the PIC by the Performance Team - Juan Cabrera

14:50 PIC input for optimization of photometric extraction algorithms - Reza Samadi

15:10 PIC: implementation and structure - Paola M. Marrese

15:30 PIC to PDC-DB and back to PSM - Cilia Damiani

15:50 From PIC to SOC to MOC to POC: the fate of PIC up to the spacecraft - Antonio Villacorta
16:10 Coffee Break
Coffee Break
16:10 - 16:35
16:35
16:35 - 17:35
Contributions

16:35 PIC update process - Silvia Marinoni

16:50 Photometric observation for PIC - Klaus Strassmeier

17:05 Synergies between the PIC and 4MOST - Roelof De Jong

17:20 Synergies between the PIC and WEAVE - Nicholas Walton
17:35
17:35 - 18:20
Contributions

17:35 PLATO fields: constraints and scientific drivers - Valerio Nascimbeni

17:50 Discussion
20:30 Social Dinner at Trattoria da Giovanni -- meeting point at 19:30 in Piazza Garibaldi
Social Dinner at Trattoria da Giovanni -- meeting point at 19:30 in Piazza Garibaldi
20:30 - 22:30
Thursday 26 September 2019
09:20
09:20 - 10:40
Contributions

09:20 Follow-up Science and PIC - Stephan Udry

09:30 A priori information for follow-up: what shall be into the PIC - Stephan Udry

09:45 Optimized follow-up scheduling - Ignasi Ribas

10:00 Gaia contribution: long-P planets for follow-up - Alessandro Sozzetti

10:15 PLATO input for ARIEL - Billy Edwards
10:40 Coffee break
Coffee break
10:40 - 11:10
11:10
11:10 - 12:00
Contributions

11:10 PIC and the PLATO World: the hard job to manage interfaces - Riccardo Claudi (Istituto Nazionale di Astrofisica (INAF))

11:20 Interfaces with WP12 - Morel Thierry

11:35 Interfaces from PSM point of view - Paul A. Wilson

11:50 Discussion
12:00

12:00 - 13:00