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Monday, June 11, 2018
| Time | Event | |
| 13:00 - 13:50 | Welcome - Welcoming session | |
| 13:50 - 14:00 | Introduction - Y.Gallant | |
| 14:00 - 14:40 | Computing accurate spectra of neutron stars for determining their parameters - F. Vincent (LUTH-Meudon) | |
| 14:40 - 15:05 | Radio observations: LOFAR and NenuFAR - J.M. Griessmeier (LPC2E-Orléans) | |
| 15:05 - 15:30 | The infancy of supernova remnants - 3D long-time simulations of SN explosions - M.Gabler (MPA-Garching) | |
| 15:30 - 15:55 | Crust-core transition in magnetars - D. Chatterjee (LPC, Caen) | |
| 15:55 - 16:30 | Coffee break | |
| 16:30 - 16:55 | HESS J1640/MSH 15-52 - M.H. Grondin (CENBG-Bordeaux)- A. Mares (CENBG-Bordeaux) | |
| 16:55 - 17:20 | The VHE gamma-ray morphology of an asymmetric pulsar wind nebula - M. Tsirou (LUPM-Montpellier) | |
| 17:20 - 17:45 | Effects of ms pulsar winds on binary companions - A.Zilles (IAP-Paris) | |
| 17:45 - 18:10 | Blind source separation methods for extended sources viewed by high energy telescopes - F.Acero (AIM-Saclay) |
Tuesday, June 12, 2018
| Time | Event | |
| 09:00 - 09:40 | Equation of state and the tidal deformability from gravitational wave measurements of LIGO and Virgo - M. Bejger (NCAC, Warsaw) | |
| 09:40 - 10:05 | Studying pulsars with DAMPE - M. Munoz Salinas (Geneva University) | |
| 10:05 - 10:40 | Coffee break | |
| 10:40 - 11:05 | Disentangling multiple high-energy emission components in the Vela X pulsar wind nebula with the Fermi Large Area Telescope - L.Tibaldo (IRAP, Toulouse) | |
| 11:05 - 11:30 | The Neutron Star Interior Composition Explorer - S.Guillot (IRAP-Toulouse) | |
| 11:30 - 11:55 | Populations of PWNe and SNRs in the HGPS - Y.Gallant (LUPM-Montpellier) | |
| 12:00 - 14:00 | Lunch | |
| 14:00 - 14:40 | New radio studies of well-known SNRs and PWNe - G.Dubner & E.Giacani (IAFE-Buenos Aires) | |
| 14:40 - 15:05 | Constraining the nature of HESS UniD - J.Devin (LUPM-Montpellier) | |
| 15:05 - 15:30 | Gamma-ray observations of star forming regions - F.Brun (CENBG-Bordeaux) | |
| 15:30 - 16:05 | Coffee break | |
| 16:05 - 16:30 | Crab Nebula - the paragon of high energy astrophysical sources - M.Lyutikov (Purdue University) | |
| 16:30 - 16:55 | Large pulsar glitch models in general relativity - J.Novak (LUTH-Meudon) | |
| 16:55 - 17:20 | The Galactic population of supernova remnant pevatrons - P.Cristofari (Columbia University) | |
| 17:20 - 17:45 | Diffusion of CRs escaping from SNRs in the atomic/molecular ISM - L.Brahimi (LUPM-Montpellier) | |
| 19:30 - 23:55 | Dinner: Le Chat Perché |
Wednesday, June 13, 2018
| Time | Event | |
| 09:00 - 09:40 | Numerical Simulations of Binary Neutron Star Mergers: Gravitational Waves and Short Gamma-Ray Bursts - B.Giacomazzo (Physics department, Trento university) | |
| 09:40 - 10:05 | A MWL view of the intriguing PWN around PSR J0855-4644 - C. Maitra (MPE-Garching) | |
| 10:05 - 10:30 | Coffee break | |
| 10:30 - 10:55 | Pevatron at the Galactic Centre: Multi-Wavelength Signatures from Millisecond Pulsars - C.Guépin (IAP-Paris) | |
| 10:55 - 11:20 | The surface emission of ms Pulsars - S.Guillot (IRAP-Toulouse) | |
| 11:20 - 11:45 | Faint gamma-ray pulsars - D.Smith (CENBG-Bordeaux) | |
| 11:45 - 11:55 | Conclusions - Y.Gallant |
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