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 |