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Contributed Paper
GP-MOOD: a positivity-preserving high-order finite volume method for hyperbolic conservation laws
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- 20 January 2023, pp. 373-379
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Hydrodynamic Simulations and Time-dependent Photoionization Modeling of Starburst-driven Superwinds
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- 20 January 2023, pp. 64-69
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Predicting the Expansion of Supernova Shells Using Deep Learning toward Highly Resolved Galaxy Simulations
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- 20 January 2023, pp. 209-214
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The non-trivial magnetic configuration in neutron stars
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- 27 February 2023, pp. 173-186
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Hydrodynamical Simulations of Misaligned Accretion Discs in Binary Systems: Companions tear discs
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- 20 January 2023, pp. 177-183
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3D Realistic Modeling of Solar-Type Stars to Characterize the Stellar Jitter
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- 20 January 2023, pp. 324-329
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Poster Paper
RNO-G detection perspectives of binary neutron star mergers
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- 27 February 2023, pp. 365-367
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Contributed Paper
The Off-Axis Afterglow of GW170817: Flux Prediction at Very High Energies
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- 27 February 2023, pp. 216-219
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Poster Paper
Improving agnostic searches of Gravitational Waves from Neutron Star instabilities using image filtering
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- 27 February 2023, pp. 352-353
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Contributed Paper
Modeling gravitational few-body problems with tsunami and okinami
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- 20 January 2023, pp. 404-409
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Velocity-space substructures and bar resonances in an N-body Milky Way
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- 20 January 2023, pp. 116-121
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X-ray Polarization at the Crossroads
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- 27 February 2023, pp. 80-91
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Inferring the dense nuclear matter equation of state with neutron star tides
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- 27 February 2023, pp. 191-194
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Poster Paper
Importance of electron-positron pairs on the maximum possible luminosity of the accretion columns in ULXs
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- 27 February 2023, pp. 327-328
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Contributed Paper
Simulating star formation in spiral galaxies
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- 20 January 2023, pp. 105-110
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Poster Paper
Detecting cosmic filamentary network with stochastic Bisous model
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- 20 January 2023, pp. 54-55
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Contributed Paper
The new magnetar SGR J1830–0645 in outburst
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- 27 February 2023, pp. 293-296
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Compact Remnant Constraints on the Core-Collapse Engine
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- 27 February 2023, pp. 19-32
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Studying Magnetic Field Amplification in Interacting Galaxies Using Numerical Simulations
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- 20 January 2023, pp. 94-99
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The formation of Supersonically Induced Gas Objects (SIGOs) with H2 cooling
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- 20 January 2023, pp. 45-50
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