Planning
| 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) |
|
| 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 |
|
| 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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