Planning
| Time |
Event |
(+)
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13:00 - 14:00
|
Welcome |
|
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14:00 - 14:10
|
Introduction - Jean-Mathias Griessmeier |
|
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14:10 - 14:45
|
Recent NICER results and constraints on the dense matter equation of state - Sébastien Guillot |
|
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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 |
|
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15:05 - 15:25
|
Unified equation of state consistent with astrophysical, gravitational, high- and low- energy nuclear physics data - Violetta Sagun |
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15:25 - 16:00
|
Coffee break |
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16:00 - 16:35
|
Modèles d'émission magnétosphérique des pulsars - Fabrice Mottez |
|
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16:35 - 16:55
|
Do Pulsars Have the same Radio Polarisation and Gamma-ray Emission Deathlines? - David Smith |
|
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16:55 - 17:15
|
Low frequency pulsar observations with NenuFAR - Louis Bondonneau |
|
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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 |
|
| 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 |
|
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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 |
|
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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 |
|
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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 |
|
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11:25 - 11:45
|
Revisiting the ejecta asymmetries in CasA with a novel method for component separation in X-rays - Adrien Picquenot |
|
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11:45 - 12:05
|
First results of the XMM Large Program on RX J1713.7-3946 - Fabio Acero |
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