General information on the School - Welcome Speech & Drink

• Nicolas Dagoneau (CEA Paris-Saclay)
• Stéphane Schanne (CEA Saclay)
• Volker Beckmann (MESR / DGRI / SSRI / A7)

Radiative processes 1/2

• Renaud Belmont (IRAP)

Active Galactic Nuclei 1/2

• Andreas Zech (LUTH - Observatoire de Paris)

Open and FAIR science

• Volker Beckmann (MESR / DGRI / SSRI / A7)

As a researcher, you are not only producing scientific articles. Most likely, you are creating valuable data sets, that could be re-used and used in a different context if available and in the right format. You might produce software that might benefit other researchers. Open and FAIR Science is the concept of sharing research results and ensuring that data are indeed FAIR, i.e. findable, accessible, interoperable, and reusable. In this lecture we explore the path to Open and FAIR Science. What does it require, what are the benefits and risks? Where can one find help and what is done at national and international level to make Open Science possible?

Welcome cocktail

• Nicolas Dagoneau (CEA Paris-Saclay)
• Stéphane Schanne (CEA Saclay)

Active galactic nuclei 2/2

• Andreas Zech (LUTH - Observatoire de Paris)

Please find my slides on the first time slot for this lecture (Wednesday, 31st May).

Radiative processes 2/2

• Renaud Belmont (CEA)

Neutrions and Cosmic-Rays

• Laurent Chevalier (CEA)

Acceleration processes 1/2

• Pierre Cristofari (Observatoire de Paris - IJCLab)

Gravitation theory 1/2

• Irina Dvorkin (Institut d'Astrophysique de Paris)

Acceleration processes 2/2

• Pierre Cristofari (Observatoire de Paris - IJCLab)

Software and development methods

• Nicolas Dagoneau (CEA Paris-Saclay)

Gravitation theory 2/2

• Irina Dvorkin (Institut d'Astrophysique de Paris)

Gravitational waves

• M. Branchesi

Breakfast at the institute Also on Sunday there is breakfast offered at the institute. But no lunch!

Gamma Ray-Bursts 1/2

• Frédéric Daigne (Institut d'Astrophysique de Paris - Sorbonne Université)

Radio Transients

• Rob Fender (University of Oxford)

Gamma Ray-Bursts 2/2

• Frédéric Daigne (Institut d'Astrophysique de Paris - Sorbonne Université)

Svom: mission and onboard prompt GRB detection

• Stéphane Schanne (CEA Saclay)

Svom: ground-based GRB follow-up observation

• Susanna Vergani (CNRS-Observatoire de Paris)

Svom: onboard GRB follow-up observation

• Diego Gotz (CEA Saclay)

General public conference in French : Quand deux étoiles à neutrons se rejoignent, ondes gravitationnelles et lumière

• Frédéric Daigne (Institut d'Astrophysique de Paris - Sorbonne Université)

General public conference (in French) La fusion de deux étoiles à neutrons est un phénomène rare mais particulièrement extrême, qui s’accompagne d’une intense émission d’ondes gravitationnelles (que l’on sait détecter depuis 2015) et de nombreux signaux lumineux, des ondes radio aux domaines infrarouge et visible et aux rayons X et gamma. Croiser ces différents signaux qui apportent des informations très complémentaires constitue une nouvelle approche très prometteuse en astrophysique. Cet exposé décrira l’émergence de cette nouvelle astrophysique multi-messagers, en particulier à travers l’exemple d’un événement exceptionnel observé en 2017.

Accretion

• Joern Wilms (Remeis Obs. & ECAP, FAU Erlangen-Nuernberg)

Neutron Stars

• Sebastien Guillot (IRAP)

X-ray Binaries 1/2

• V. Grinberg

X-ray high resolution spectroscopy

• Joern Wilms (Remeis Obs. & ECAP, FAU Erlangen-Nuernberg)

X-ray Binaries 2/2

• V. Grinberg

Optical transients with LSST and Fink

• Damien TURPIN (CEA-Saclay)

Barbecue

Svom: Demonstration of Burst-Advocates' tools

• Damien TURPIN (CEA-Saclay)