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CONFERENCE POSTERS
Session 1: Populations/Surveys and Classifications of SNRs and SNe
| S1.1 | F. Bocchino | GalRSG: A long-term monitoring campaign of Galactic Red Supergiants and the quest for SN explosions’ premonitory signs |
| S1.2 | F. Bocchino | Search for Gamma-ray emission from SNRs in the Large Magellanic Cloud: Preliminary results of a new cluster analysis at energies above 3GeV |
| S1.3 | C. Burger-Scheidlin | Gamma-ray detection of newly discovered Ancora supernova remnant: G288.8–6.3 |
| S1.4 | A. Castrillo | Supernova remnant catalog in the PHANGS survey |
| S1.5 | M. Filipovic | Mysterious Odd Radio Circle near the Large Magellanic Cloud – An Intergalactic Supernova Remnant? |
| S1.6 | B. Gamache | Characterization of M51 supernovae remnants with the imaging spectrometer SITELLE |
| S1.7 | D. A. Green | Statistics of Galactic Supernova Remnants |
| S1.8 | A. Ingallinera | Studying SNRs and their environment with high-resolution radio spectral index maps |
| S1.9 | A. Khokhriakova | SNR G321.3-3.9 observed with multi-band radio data and SRG/eROSITA |
| S1.10 | I. Leonidaki | Disentangling the evolutionary paths of Supernova Remnants: observational evidence of (non) multi-wavelength emission |
| S1.11 | I. Leonidaki | A systematic meta-analysis of physical parameters of Galactic SNRs |
| S1.12 | T.-X. Luo | Investigation of Galactic supernova remnants and their environment in 26.6°<l<30.6°, |b|≤ 1.25° using radio survey |
| S1.13 | S. Mantovanini | Low radio frequency images of the southern Galactic plane for supernova remnant detection |
| S1.14 | M. Michailidis | X-ray counterpart detection and gamma-ray analysis of the SNR G279.0+01.1 with eROSITA and Fermi-LAT |
| S1.15 | K. Ronald | An L-band Panoramic View of Galactic Supernova Remnants with the Australian SKA Pathfinder |
| S1.16 | S. Panjkov | The Core-Collapse Progenitor Mass Distribution of the Large Magellanic Cloud |
| S1.17 | N. O. Pinciroli Vago | DeepGraviLens: a multi-modal architecture for classifying gravitational lensing data |
| S1.18 | Z. Smeaton | Discovery of new, young Galactic SNR (G329.9-0.5) |
Session 2: SNe and SNRs with Circumstellar Interactions
| S2.1 | M. Arias | Probing supernova remnant VRO 42.05.01’s progenitor properties with IRAM 30m observations |
| S2.2 | R. Baer-Way | A multi-wavelength autopsy of a young interacting supernova to unveil its progenitor |
| S2.3 | M. Chatzopoulos | Radiative Transfer Modeling of Astrophysical Transients Powered by Circumstellar Interaction |
| S2.4 | W.-Y. Chen | Multidimensional Radiation Hydrodynamics Simulations of Supernova 1987a Shock Breakout |
| S2.5 | W.-Y. Chen | 2D Rad-Hydro Shock Breakout Simulations on RSG with CSM |
| S2.6 | A. Chrimes | Clues (and conunumdrums) from the circumstellar media around extreme extragalactic transients |
| S2.7 | T. Court | Type Ia Supernova Remnants in Different Circumstellar Environments |
| S2.8 | J. Horvat | An XMM-Newton study of several nonradiative filaments in the northeastern rim of the Cygnus Loop |
| S2.9 | M. Ichihashi | The thermal relaxation process in collisionless shock of SN1006 |
| S2.10 | W. Jacobson-Galan | Final Moments: Observational Properties and Physical Modeling of “Flash Spectroscopy” Supernovae |
| S2.11 | B. Liu | Investigation into SNR-accelerated CRs at the prospect of future MeV gamma-ray detectors |
| S2.12 | L.-D. Liu | Light curves of Multiple Ejecta-circumstellar Medium Interactions |
| S2.13 | E. Makarenko | Thermal X-ray emission from supernova remnants in 3D (M)HD simulations |
| S2.14 | M. Matsuura | Infrared emission of supernova remnants in the Small Magellanic Cloud |
| S2.15 | A. Mercuri | Spectral Analysis of Chandra data on selected regions of the Supernova Remnant Cassiopeia A |
| S2.16 | T. Murase | Molecular Clouds associated with middle-aged gamma-ray Supernova Remnants W41 and G22.7–0.2 |
| S2.17 | A. Nagy | How can circumstellar interaction explain the special light curve features of Type Ib/c supernovae? |
| S2.18 | S. Orlando | Constraining the CSM structure and progenitor mass-loss history of SN 2014C through 3D hydrodynamic modeling |
| S2.19 | B. H. Pál | A possible circumstellar interaction of SN2004gq |
| S2.20 | O. Petruk | Density and magnetic field gradients in Tycho SNR |
| S2.21 | G. Prete | Interaction of a Supernova Remnant with background interstellar turbulence |
| S2.22 | L. Sun | Probe charge exchange and resonant scattering in Magellanic Cloud supernova remnants with spatially-resolved high-resolution X-ray spectroscopic study of oxygen lines |
| S2.23 | I. Sushch | Role of reflected shocks in particle acceleration in supernova remnants |
| S2.24 | A. Suzuki | Multi-dimensional simulations of interaction-powered supernovae |
| S2.25 | H. Suzuki | Global and Rapid Deceleration of X-Ray Knots and Rims of RCW 103 |
| S2.26 | K. Tsuge | Shocked Molecular Clouds in the LMC SNR N132D Revealed by ALMA ACA |
| S2.27 | S. Ustamujic | Modeling the mixed-morphology supernova remnant VRO 42.05.01 |
Session 3: SN/SNR Progenitors, Central Engines, Explosion Models
| S3.1 | E. Abdikamalov | Exploring supernova gravitational waves with machine learning |
| S3.2 | M. Anazawa | Estimation of progenitor of Keplers SNR with precision X-ray spectroscopic analysis |
| S3.3 | B. Arbutina | Modeling Binary Systems That Survive Supernova Explosions and Give Rise to Gravitational Waves |
| S3.4 | B. Barna | Different, but still same: on the common(?) origin of the peculiar Type Iax SNe |
| S3.5 | E. Batziou | The Long-time Evolution of Accretion-Induced Collapse of White Dwarfs to Neutron Stars |
| S3.6 | Z. R. Bodola | Massive Progenitor Parade of Stripped-Envelope Supernovae |
| S3.7 | A. Z. Bonanos | Evidence for episodic mass loss in red supergiants from the ASSESS project |
| S3.8 | K. A. Bostroem | Considering the Single and Binary Origins of the Type IIP SN 2017eaw |
| S3.9 | M. Bugli | Numerical models of magneto-rotational supernovae: dynamics, multi-messenger signals, and explosive nucleosynthesis |
| S3.10 | M. Bugli | 3D MHD core-collapse supernovae code comparison: the impact of numerics on central engine’s simulations |
| S3.11 | E. Christodoulou | Obtaining accurate parameters of Type IIP progenitors in NGC 6822, IC 10 & WLM |
| S3.12 | L. Dang | Typing supernova remnant G352.7−0.1 using XMM-Newton X-ray observations |
| S3.13 | B. Dinçel | Possible pre-supernova binary companion to the progenitor of the supernova remnant IC 443 |
| S3.14 | O. Eggenberger Andersen | Black Hole Supernovae and their Equation-of-state Dependence |
| S3.15 | J. I. Gonzalez-Hernandez | Searching for surviving stellar companions of historical galactic type Ia supernovae |
| S3.16 | A. Holas | Electron-capture supernovae – Thermonuclear explosion or gravitational collapse? – The fate of sAGB stars on a knife’s edge |
| S3.17 | C. M. Irwin | An unexplored regime of shock breakout: the effect of rapid thermalization on the observed spectrum |
| S3.18 | M. Kalitsounaki | Discovery of an extreme Red Supergiant in the LMC transitioning to a Blue Supergiant |
| S3.19 | E. Kasdagli | Improving Supernova Prescriptions in Binary Population Synthesis Using Detailed Stellar Profiles |
| S3.20 | J. Luo | 3D Simulation of SN~Ia SNR: Effects of Companion Star and Progenitor System |
| S3.21 | K. Matsunaga | Formation of Mg-rich SNRs by shell merger and its effect on the explodability |
| S3.22 | G. Munoz-Sanchez | [W60] B90: a mass-losing luminous RSG in the LMC interacting with the CSM |
| S3.23 | T. Narita | Progenitor constraint with CNO abundances of circumstellar material in supernova remnants |
| S3.24 | Z. Niu | The binary progenitor for Type IIP supernovae |
| S3.25 | C. Omand | Probing Energetic Infant Pulsars with Supernova Emission Lines |
| S3.26 | K.-C. Pan | Stellar Mass Black Hole Formation and Multimessenger Signals from Core-collapse Supernova Simulations |
| S3.27 | G. Pignata | Three years observations of the nearby type II SN2008bk |
| S3.28 | A. Rest | The Historic Light Curve of Eta Car’s Great Eruption from its Light Echoes |
| S3.29 | P. Ruiz-Lapuente | SN Ia supernova remnant with M dwarf companions |
| S3.30 | R. Sawada | ‘56Ni problem’ in Canonical Supernova Explosion |
| S3.31 | M. Shahbandeh | The Life Story of Stripped-Envelope Supernovae as told through JWST Observations |
| S3.32 | M. Solar | Binary progenitor systems for Type Ic supernovae |
| S3.33 | T. Tanaka | Expansion Measurements of Tycho’s Supernova Remnant and Their Implications of the Progenitor System |
| S3.34 | H. Uchida | Possible evidence of a jet-induced explosion found from X-ray and radio observations of a peculiar SNR G0.61+0.01 |
| S3.35 | J. Weng | Upper Limits of 44Ti Decay Emission in Four Nearby Thermonuclear Supernova Remnants |
Session 4: SNR Structure, Ejecta and Evolution
| S4.1 | M. Agarwal | X-ray diagnostics of Cassiopeia A’s “Green Monster”: evidence for dense shocked circumstellar plasma |
| S4.2 | S. Akras | Spectroscopic analysis tool for intEgraL fieLd unIt daTacubEs (SATELLITE): The case of SNR 0509-68.7 |
| S4.3 | M. Anđelić | On the origin of the North Polar Spur |
| S4.4 | Y. Chen | A Monte-Carlo Simulation on Resonant Scattering of X-ray Line Emission in Supernova Remnants |
| S4.5 | Y.-H. Chi | Thermal X-ray Emission in the Western Half of the LMC Superbubble 30 Dor C |
| S4.6 | P. Das | Integral field spectroscopy of type Ia supernova remnants. |
| S4.7 | D. Dickinson | High Resolution Mapping of the Unshocked Ejecta in Cassiopeia A |
| S4.8 | M. Fontaine | Theoretical and Experimental Simulations of Colliding Blast Waves |
| S4.9 | B. Giudici | Hydrodynamic instabilities in three-dimensional simulations of neutrino-driven supernovae of 14 red supergiant progenitors |
| S4.10 | R. Giuffrida | Measuring the initial mass of 44Ti in SN 1987A through the 44Sc emission line |
| S4.11 | L. Godinaud | Mapping the 3D dynamics and spectral properties of Tycho’s SNR in X-rays |
| S4.12 | T. Ko | The multi-layer structure of SNR 1181 with a white dwarf in its center |
| S4.13 | B.-C. Koo | JWST Observations of the Cassiopeia A Supernova Remnant: Near-Infrared Colors of Supernova Ejecta |
| S4.14 | D. Leahy | On emission measures and element densities and masses inferred from XSPEC |
| S4.15 | D. Leahy | Models for supernova remnants with reverse shock emission |
| S4.16 | E. Makarenko | How do supernova remnants cool? Morphology and optical emission lines |
| S4.17 | S. Mandal | Measurement of anisotropies in observed Supernova Remnants and their interpretation using hydrodynamical models |
| S4.18 | M. Ono | Molecular formation in the ejecta of SN 1987A based on three-dimensional hydrodynamical models |
| S4.19 | S. Panjkov | Morphological Insights into the SN progenitors of the Small Magellanic Cloud |
| S4.20 | G. Paylı | Investigation of supernova remnant IC 443 and G189.6+3.3 with LAMOST |
| S4.21 | L. Romano | Cloud Formation by Supernova Implosion |
| S4.22 | V. Sapienza | Probing Shocked Ejecta in SN 1987A: A novel diagnostic approach using XRISM-Resolve |
| S4.23 | N. Sanches Sartorio | New Analytical Solutions for Supernova Shocks |
| S4.24 | S. Sarbadhicary | Anatomy of a shock: IFU map of RCW86 with the SDSS-V Local Volume Mapper |
| S4.25 | L. Sun | Evolution of X-ray Gas in SN 1987A from 2007 to 2021: Ring Fading and Ejecta Brightening Unveiled through Differential Emission Measure Analysis |
| S4.26 | J. C. Toledo-Roy | Simulated non-thermal emission of the supernova remnant G1.9+0.3 |
| S4.27 | D. Urošević | A method for determination of evolutionary status of supernova remnants from radio data |
| S4.28 | B. van Baal | Nebular Phase Stripped Envelope Supernovae in 3D |
| S4.29 | K. Vargas Rojas | Study of non-thermal emission of Kepler’s SNR with MHD numerical simulations. |
Session 5: Shock Physics, Particle Acceleration, Polarization in SNRs and PWNe
| S5.1 | F. Acero | How I learned to stop trusting my X-ray spectral best fits and love nested sampling |
| S5.2 | B. Ball | Radio Polarization Studies of Galactic Supernova Remnants with ASKAP |
| S5.3 | D. Castro | The Expansion and Width of the Synchrotron Filaments Associated with the Forward Shocks of SNRs |
| S5.4 | L. Del Zanna | Relativistic MHD turbulence simulations and synchrotron polarization properties of Pulsar Wind Nebulae |
| S5.5 | R. Ferrazzoli | X-ray polarimetry of RX J1713.7-394 |
| S5.6 | R. Giuffrida | Evidence for proton acceleration and escape from the Puppis A SNR using Fermi-LAT observations |
| S5.7 | E. Greco | Jitter radiation as an alternative mechanism for the nonthermal emission in Cassiopeia A |
| S5.8 | J. Hewitt | Resolving the gamma-ray supernova remnant IC 443 with Fermi LAT and VERITAS |
| S5.9 | J. Hewitt | Two new radio-dim, gamma-ray-bright supernova remnants |
| S5.10 | S. Knežević | Shock geometry and physics in the supernova remnant SNR 0509-67.5 |
| S5.11 | P. Kostić | Kinetic-based CFD modeling of synchrotron emission spectra at fast SNRs |
| S5.12 | Y. Ohshiro | A self-consistent model of shock-heated plasma in non-equilibrium states for direct parameter constraints from X-ray observations |
| S5.13 | V. Sapienza | Polarization and time evolution of the synchrotron emission in Kepler’s SNR |
| S5.14 | X. Shi | The production of unstable cosmic-ray isotopes in supernovae clusters |
| S5.15 | J. D. Slavin | Modeling Shock Emission Including Dust Destruction |
| S5.16 | K. Stasiewicz | Reinterpretation of the Fermi acceleration of cosmic rays in terms of the ballistic surfing acceleration in supernova shocks |
| S5.17 | S. J. Tanaka | A Self-regulated Stochastic Acceleration Model of Pulsar Wind Nebulae |
| S5.18 | D. Tateishi | Suzaku/XIS study of the acceleration environment of bilateral SNR RX J0852.0-4622 |
| S5.19 | S. Ustamujic | Modeling the supernova remnant RX J1713.7 – 3946: particle acceleration, gamma-ray emission, and neutrino flux |
Session 6: SN/SNR dust, environments, feedback
| S6.1 | E. Chatzopoulos | Stellar Alchemy: 3D Mergers As Sources of Circumstellar Material Around SN Progenitors |
| S6.2 | E. Dwek | The evolution and origin of the infrared emission from SN2010jl |
| S6.3 | N. Izumi | CI/CO abundance ratio of shock-excited gas in the Magellanic Supernova Remnant N63A |
| S6.4 | F. Kirchschlager | Dust destruction in the clumpy remnant Cassiopeia A: impact of inhomogeneous dust distributions |
| S6.5 | N. Sanches Sartorio | The impact of CSM properties on the dust destruction by supernovae forward shocks |
| S6.6 | H. Sano | ALMA Observations of Supernova Remnant N49 in the Large Magellanic Cloud. II. Non-LTE Analysis of Shock-heated Molecular Clouds |
| S6.7 | T. Scheffler | Dust destruction by supernova remnant forward shocks in a turbulent interstellar medium |
| S6.8 | A. Singleton | Constraining the progenitor properties of the Type Ib supernova iPTF13bvn through its environment with HST and MUSE |
| S6.9 | D. Souropanis | Time-dependent feedback of core-collapse supernovae from binary progenitors via detailed binary population synthesis models |
| S6.10 | T. Tu | A Yebes W band Line Survey towards an Unshocked Molecular Cloud of Supernova Remnant 3C391: Evidence of Cosmic-Ray-Induced Chemistry |
| S6.11 | R. Wesson | The slow formation of dust by core collapse supernovae |
| S6.12 | M. Zhang | Not gone with the wind: survival of high-velocity molecular clouds in the Galactic Centre |
| S6.13 | Q. Zhang | A molecular line survey toward clumps G and E in supernova remnant IC 443 with the Submillimeter Array |
| S6.14 | Z. Zhang | Estimation of the Dust Mass with Infrared Emission and Extinction of the Supernova Remnants: G156.2+5.7, G109.1-1.0, G166.0+4.3, G93.7-0.2 |
| S6.15 | S. Zsíros | Disentangling possible dust components of core-collapse supernovae within a Bayesian framework |
Session 7: PWN Diversity; Structures, Bowshocks and Magnetar Wind Nebulae
| S7.1 | J. Alford | Cosmic Ray Leptons Escaping from CTA 1? |
| S7.2 | Y. Chen | “Mirage” and large offsets in the data as a result of asymmetric CR diffusion |
| S7.3 | L. V. da Conceição | Using CFHT’s SITELLE to probe the long-sought shell in the Crab nebula |
| S7.4 | S. Gagnon | Chandra X-ray Observations of PSR J1849-0001 and its Pulsar Wind Nebula |
| S7.5 | X. Li | An Exploration of Misaligned Outflows in Pulsar Wind Nebulae |
| S7.6 | S. Mandal | Diagnosis of Pulsar Wind Nebula dynamics using their filamentary structure |
| S7.7 | K. Yan | Pulsar halos as an origin of the Galactic diffuse TeV-PeV emission: Insight from LHAASO and IceCube |
Session 8: SNRs and PWNe as PeVatrons
| S8.1 | R. Brose | Fast Blue Optical Transients as cosmic-ray sources |
| S8.2 | R. Diesing | The Maximum Energy of Shock-Accelerated Cosmic Rays |
| S8.3 | Y. Gallant | Pulsar Wind Nebulae and their halos observed in TeV and PeV gamma rays |
| S8.4 | S. Lazarevic | Radio-continuum view of PeVatrons |
| S8.5 | Y. Li | Multi-Messenger Modeling of the Monogem Pulsar Halo |
| S8.6 | B. Mac Intyre | The Manatee Nebula W50-SS433: a Galactic PeVatron? |
| S8.7 | I. Sander | Pulsar Wind Nebulae and PeVatrons: A Case Study of PWN G309.92-2.51 |
| S8.8 | N. Tsuji | Search for molecular clouds associated with PeVatrons by the Nobeyama 45-m radio telescope: the case of LHAASO J0341+5258 |
Session 9: SNR/PWN/Compact Objects Associations, Interaction and Evolution
| S9.1 | J. Ahlvind | Late-time X-ray observations Core-Collapse Supernovae – constraints on emission from compact objects and CSM interaction |
| S9.2 | T. Kravtsov | Discovery of new oxygen-rich supernova remnants |
| S9.3 | A. M. Moaz | Multi-Wavelength Modelling of the Pulsar Wind Nebulae Kes 75 & HESS J1640-465 |
| S9.4 | J. Suherli | A-MUSE-ing Views of the Central Environment of the Vela Jr. and 1E0102-72.3 Supernova Remnants |