Missing data in physics - Sciencesconf.org

›9:15 (15min)

Registration

9:15 - 9:30 (15min)

Registration

›9:30 (10min)

Welcome
J. Bergé / S. Pires

› Cézanne

9:30 - 9:40 (10min)

Welcome

Cézanne

J. Bergé / S. Pires

›9:40 (1h05)

Handling missing data with sparse and low-rank models
J. Bergé

› Cézanne

9:40 - 10:45 (1h05)

Handling missing data with sparse and low-rank models

Cézanne

J. Bergé

› Ten years later - Jean-Luc Starck, CEA Saclay 09:40-10:20 (40min)

› Point spread function field interpolation using optimal transport - NGOLE MBOULA Fred Maurice, Service d'Astrophysique 10:20-10:45 (25min)

›10:45 (30min)

Coffee break

10:45 - 11:15 (30min)

Coffee break

›11:15 (1h15)

Equivalence Principle measurement with Microscope
S. Pires

› Cézanne

11:15 - 12:30 (1h15)

Equivalence Principle measurement with Microscope

Cézanne

S. Pires

› The MICROSCOPE mission to test the Equivalence Principle in space - Gilles METRIS, Observatoire de la Côte d'Azur 11:15-11:40 (25min)

› MICROSCOPE data processing and analysis, missing data and inpainting - Joel Bergé, Département de Mesures Physiques 11:40-12:05 (25min)

› In-orbit test of the equivalence principle with MICROSCOPE : the missing data challenge - Quentin Baghi, ONERA 12:05-12:30 (25min)

›12:30 (2h)

Lunch

12:30 - 14:30 (2h)

Lunch

›14:30 (1h15)

Geoscience data
G. Métris

› Cézanne

14:30 - 15:45 (1h15)

Geoscience data

Cézanne

G. Métris

› Impact of the twangs on the GRACE data recovery - Bernard Foulon, Onera - The French Aerospace Lab 14:30-14:55 (25min)

› Seismo-ionospheric disturbances sensing using GPS data: catching the seismic wavefield from space - Lucie Rolland, Géoazur 14:55-15:20 (25min)

› SIRTA-ReOBS: the multi-parameter homogenized and value-added database of the SIRTA observatory in Paris region. - Jordi Badosa, Laboratoire de Météorologie Dynamique 15:20-15:45 (25min)

›15:45 (50min)

Gravitational waves detection technology demonstration with LISA Pathfinder
B. Foulon

› Cézanne

15:45 - 16:35 (50min)

Gravitational waves detection technology demonstration with LISA Pathfinder

Cézanne

B. Foulon

› The LisaPathfinder Mission - Eric Plagnol, AstroParticule et Cosmologie 15:45-16:10 (25min)

› LISA Pathfinder Data Analysis - Martin Hewitson, University of Hannover 16:10-16:35 (25min)

›16:35 (30min)

Coffee break

16:35 - 17:05 (30min)

Coffee break

›17:05 (50min)

Stochastic data
E. Plagnol

› Cézanne

17:05 - 17:55 (50min)

Stochastic data

Cézanne

E. Plagnol

› Reconstruction of turbulent flows from partial measurements and statistics - Berengere Podvin, LIMSI-CNRS 17:05-17:30 (25min)

› Influence of irregular node spacing in noisy rational interpolation. - Jean Fournier, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux 17:30-17:55 (25min)

›20:00 (2h)

Dinner

20:00 - 22:00 (2h)

Dinner