Monday, April 8, 2019

Time Event  
13:00 - 14:00 Welcome  
14:00 - 14:10 Introduction - Jean-Mathias Griessmeier  
14:10 - 14:45 Recent NICER results and constraints on the dense matter equation of state - Sébastien Guillot
 
14:45 - 15:05 New constraints on the equation of state of dense nuclear matter using thermal emission of neutron stars - Nicolas Baillot d'Etivaux
 
15:05 - 15:25 Unified equation of state consistent with astrophysical, gravitational, high- and low- energy nuclear physics data - Violetta Sagun
 
15:25 - 16:00 Coffee break  
16:00 - 16:35 Modèles d'émission magnétosphérique des pulsars - Fabrice Mottez
 
16:35 - 16:55 Do Pulsars Have the same Radio Polarisation and Gamma-ray Emission Deathlines? - David Smith
 
16:55 - 17:15 Low frequency pulsar observations with NenuFAR - Louis Bondonneau
 
17:15 - 17:35 Constraining galaxy and black hole binary mergers with pulsars - Siyuan Chen
 
17:35 - 17:55 Impacts of planetary ephemerides on Pulsar Timing Arrays results - Aurélien Chalumeau
 

Tuesday, April 9, 2019

Time Event  
09:00 - 09:35 A Review of the Spider Pulsar Population - René Breton  
09:35 - 09:55 X-ray observations of Spiders - Mallory Roberts  
09:55 - 10:15 Nancay Radio Telescope discovery of the eclipsing black widow pulsar PSR J2055+3829 - Lucas Guillemot
 
10:15 - 10:45 Coffee break  
10:45 - 12:00 The future of MODE SNR-PWN workshops - Plenary discussion  
12:00 - 14:00 Lunch  
14:00 - 14:35 X-raying nearby thermal and non-thermal remnants : The case of Magellanic supernova remnants, superbubbles, and pulsar wind nebulae - Pierre Maggi
 
14:35 - 14:55 The population of PWNe seen by HESS and their Galactic environments - Yves Gallant
 
14:55 - 15:15 A deep look at the HESS J1825-137 pulsar wind nebula with H.E.S.S. and Fermi-LAT - Sami Caroff
 
15:15 - 15:35 Efficient particle acceleration from HESS J1640.6-4633 and the PeVatron candidate HESS J1641.0-4619 - Arnaud Marès
 
15:35 - 15:55 Is G150.3+4.5 old or one of the closest GeV gamma-ray SNRs ? - Justine Devin
 
15:55 - 16:30 Coffee break  
16:30 - 16:50 Towards a better understanding of dense matter with gravitational waves - Jérôme Margueron
 
16:50 - 17:10 Constraints on Dense Matter Equation of State from GW170817: Possibility of Different Families of Compact Stars - Prasanta Char
 
17:10 - 17:30 The stability properties of differentially rotating neutron stars - Pawel Szewczyk
 
17:30 - 17:50 Neutron star properties from an extended linear sigma model - János Takátsy
 

Wednesday, April 10, 2019

Time Event  
09:00 - 09:35 An observational overview on highly magnetic neutron stars - Francesco Coti-Zelati
 
09:35 - 09:55 Glitch Behavior of Pulsars and Contribution from Neutron Star Crust - Avishek Basu  
09:55 - 10:15 Assessing the evidence of multipolar fields in pulsars - Prakash Arumugasamy
 
10:15 - 10:45 Coffee break  
10:45 - 11:05 Stellar and interstellar content of the region interacting with cosmic rays in IC443 - Pierre Dell'ova
 
11:05 - 11:25 Gamma-ray emission from supernova remnants interacting with interstellar clouds - Jean Ballet
 
11:25 - 11:45 Revisiting the ejecta asymmetries in CasA with a novel method for component separation in X-rays - Adrien Picquenot
 
11:45 - 12:05 First results of the XMM Large Program on RX J1713.7-3946 - Fabio Acero