A | B | C | D | E | F | G | H | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z | |
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1 | Board Number | First Name | Last Name | Poster Title | ||||||||||||||||||||||
2 | in person | |||||||||||||||||||||||||
3 | 1 | Tomotada | Akutsu | Commissioning with machine learning: regression analysis for alignment errors in the KAGRA interferometer | ||||||||||||||||||||||
4 | 2 | Christopher | Alléné | Early Warning Study : Intersearch Coincidences | ||||||||||||||||||||||
5 | 3 | Sama | Al-Shammari | Machine learning for parameter estimation of Gravitational waves data towards waveform systematics | ||||||||||||||||||||||
6 | 4 | Marc | Andrés-Carcasona | Scattered Light in the Main Arms of ET | ||||||||||||||||||||||
7 | 5 | Tomislav | Andric | First demonstration of neural sensing and control in a kilometer-scale gravitational wave observatory | ||||||||||||||||||||||
8 | 6 | Scott | Aronson | Quantum Optics at LSU | ||||||||||||||||||||||
9 | 7 | Rishabh | Bajpai | Estimating Newtonian noise of KAGRA Cryostat | ||||||||||||||||||||||
10 | 8 | Freija | Beirnaert | A Study of the Large Scale Structure of the Universe using Gravitational Waves | ||||||||||||||||||||||
11 | 9 | Marceline | Bonilla | Rescaled ppE Parameters for Parameter Estimation Across Fractional PN Order | ||||||||||||||||||||||
12 | 10 | Matteo | Carlassara | Balanced Homodyne Detection at the AEI 10 m prototype: status update | ||||||||||||||||||||||
13 | 11 | Ruei-Jhe | Chang | Performance test of CBC classification via deep learning | ||||||||||||||||||||||
14 | 12 | Andy | Chen | False Alarm Rate reduction for unknown Core-Collapse Supernova detection via Machine Learning | ||||||||||||||||||||||
15 | 13 | Anson | Chen | Testing gravity using dark sirens and galaxy catalogues | ||||||||||||||||||||||
16 | 14 | Dan | Chen | Photon Calibration System for KAGRA O4 | ||||||||||||||||||||||
17 | 15 | Damon, Hoi Tim | Cheung | Mitigating the effect of population model uncertainty on strong lensing Bayes factor using non-parametric methods | ||||||||||||||||||||||
18 | 16 | Taishi | Sako | About High Power Laser Systems at KAGRA | ||||||||||||||||||||||
19 | 17 | Gabriella | Chiarini | Mode mismatch sensing through RF Higher Order Modulation | ||||||||||||||||||||||
20 | 18 | Ayuto | Chiba | Installation and environmental noise measurement of optical lever for KAGRA cryogenic payload | ||||||||||||||||||||||
21 | 19 | Chia-Jui | Chou | Demonstration of Machine Learning-assited real-time noise regression in GW detectors | ||||||||||||||||||||||
22 | 20 | Sunil | Choudhary | Improvements to SPIIR pipeline in O4 | ||||||||||||||||||||||
23 | 21 | Teagan | Clarke | Exploring a coincident FRB and sub-threshold NSBH merger during O3b | ||||||||||||||||||||||
24 | 22 | Weichangfeng | Guo | P Astro: GW Trigger Classification for SPIIR Pipeline | ||||||||||||||||||||||
25 | 23 | Paolo | Cremonese | Mass-Sheet Degeneracy in Gravitational Wave Microlensing | ||||||||||||||||||||||
26 | 24 | Aaron | Davenport | Current Development of High Reflection TiO2:GeO2 and SiO2 Coatings for Gravitational Wave Detectors | ||||||||||||||||||||||
27 | 25 | Diego | Dominguez | Convolutional Neural Network for continuous gravitational waves detection | ||||||||||||||||||||||
28 | 26 | Jose Maria | Ezquiaga | Identifying strongly lensed gravitational waves through their phase consistency | ||||||||||||||||||||||
29 | 27 | Giulio | Favaro | Effects of partial crystallization on coating internal friction in ion-beam sputtered Ta2O5 thin films | ||||||||||||||||||||||
30 | 28 | Subham | Vidyant | FPGA based Phase Camera Update | ||||||||||||||||||||||
31 | 29 | Takumi | Fujimori | Analysis of the motion of the Sun as seen from the Earth | ||||||||||||||||||||||
32 | 30 | Suyog | Garg | Deep Convolutional Neural Network for detecting Gravitational Wave signals from Eccentric Compact Binaries | ||||||||||||||||||||||
33 | 31 | Jane | Glanzer | Investigations of Binary Neutron Star Range Oscillations at LIGO Livingston | ||||||||||||||||||||||
34 | 32 | Shingo | Fujii | Calibration of the integrating sphere for O4 in KAGRA gravitational wave telescope | ||||||||||||||||||||||
35 | 33 | Jaxen | Godfrey | Population source characterization with astrophysical mixture models | ||||||||||||||||||||||
36 | 34 | Yi | GONG | Including higher harmonics in gravitational-wave parameter estimation for LISA | ||||||||||||||||||||||
37 | 35 | Graziano | Pascale | Laser power stabilization via radiation pressure | ||||||||||||||||||||||
38 | 36 | Andre | Guimaraes | Characterizing the Behavior of CBC Search Pipelines in Response to Noise Transients in the aLIGO Detector | ||||||||||||||||||||||
39 | 37 | Reiko | Harada | Examination of the Testability of the Quark-Hadron Transition Using Gravitational Waves From Merging Binary Neutron Stars | ||||||||||||||||||||||
40 | 38 | HsienYi | Hsieh | Extract correlation functions among degradation sources in frequency-dependent squeezed vacuum source with neural network | ||||||||||||||||||||||
41 | 39 | Hsiang-Chieh | Hsu | Study of the cryogenic system and active vibration isolation system for gravitational wave detection | ||||||||||||||||||||||
42 | 40 | dven | Hui | Improving Detection/Classification of Gravitational Wave Signal by Generative Adversarial Network (GAN) | ||||||||||||||||||||||
43 | 41 | Hayato | Imafuku | Search for scalar polarization of gravitational waves | ||||||||||||||||||||||
44 | 42 | Masaki | Iwaya | Constraining the extremely metal-poor BBH formation scenario using GWTC-3 | ||||||||||||||||||||||
45 | 43 | Shreejit | Jadhav | Towards a robust deep learning model for gw searches | ||||||||||||||||||||||
46 | 44 | Wasim | Javed | Robust sky localisation technique for GW burst signals in low latency search using Coherent Null-Stream analysis | ||||||||||||||||||||||
47 | 45 | Nicholas | Johnson | Thermo-Optical Measurements of KTF and TGG Crystals as Faraday Isolator Materials | ||||||||||||||||||||||
48 | 46 | Kihyun | Jung | Classification and Analysis of KAGRA Glitches using Hveto during O3GK | ||||||||||||||||||||||
49 | 47 | Izumi | Kaku | Simulation analysis in gravitational wave radiometry introducing Stokes parameter | ||||||||||||||||||||||
50 | 48 | Purnendu | Karmakar | Testing Non-metricity Geometry | ||||||||||||||||||||||
51 | 49 | Jumpei | Kato | Laser Intensity Stabilization system of KAGRA for 04 | ||||||||||||||||||||||
52 | 50 | Takashi | Kato | Detectability of CBC GW events with KAGRA at O4b | ||||||||||||||||||||||
53 | 51 | JeongCho | Kim | Sampling method to determine eccentricity using TaylorF2Ecc | ||||||||||||||||||||||
54 | 52 | Minhyo | Kim | Atomic structure characterization study on optimization of TiO2-doped GeO2 material for reducing coating Brownian noise | ||||||||||||||||||||||
55 | 53 | Sangin | Kim | Autoregressive Search of Gravitational Waves | ||||||||||||||||||||||
56 | 54 | Young-Min | Kim | Bayesian Inference of Neutron Star Equation of State with KIDS density functionals | ||||||||||||||||||||||
57 | 55 | Nicole | Knust | A Pre-Stabilized 1550 nm Laser Source for the ETpathfinder | ||||||||||||||||||||||
58 | 56 | Kai-Yu | LIN | The Gravity Realm: exhibition at the National Museum of Natural Science, Taiwan | ||||||||||||||||||||||
59 | 57 | You-Ru | Lee | Exploration of O5 Sensing Function with Balanced Homodyne Readout for Calibration in LIGO | ||||||||||||||||||||||
60 | 58 | Samson | Leong | Improving the coincidence of BBH with EM counterpart from AGN with measurement of remnant BH kick | ||||||||||||||||||||||
61 | 59 | Alvin Ka Yue | Li | "What does a car has to do with targeted lensing searches?" - The TESLA trilogy | ||||||||||||||||||||||
62 | 60 | Manoj | Kovalam | SPIIR Low Latency Pipeline | ||||||||||||||||||||||
63 | 61 | Yannick | Lecoeuche | Evaluating the effects of glitches on compact binary coalescence parameter estimation | ||||||||||||||||||||||
64 | 62 | Suprovo | Ghosh | Tidal heating as a direct probe of Strangeness inside Neutron stars | ||||||||||||||||||||||
65 | 63 | Yu-Chiung | Lin | Extracting Gravitational Wave Feature Using Self-Supervised Learning Denoiser | ||||||||||||||||||||||
66 | 64 | Alexandre | Lussier | Effects of bond passivating dopants in a-Si on its optical properties | ||||||||||||||||||||||
67 | 65 | Elisa | Maggio | Mock data challenge for tests of general relativity: the pSEOBNRv4HM_PA pipeline | ||||||||||||||||||||||
68 | 66 | Mahoro | Matsuyama | Tidal deformability estimation using Machine Learning | ||||||||||||||||||||||
69 | 67 | Breck | Meagher | SEM Imaging of GaAs/AlGaAs Crystalline Coatings | ||||||||||||||||||||||
70 | 68 | Kara | Merfeld | A coherent pipeline to perform stacked searches on repeated EM bursts | ||||||||||||||||||||||
71 | 69 | Soichiro | Morisaki | Rapid and automated parameter estimation on compact binary coalescences in O4 | ||||||||||||||||||||||
72 | 70 | Kouji | Nakamura | Quantum noise and vacuum fluctuationsin balanced homodyne detections through ideal multi-mode detectors | ||||||||||||||||||||||
73 | 71 | Debasmita | Nandi | Hunting the Scattered Light Noise in LIGO Livingston | ||||||||||||||||||||||
74 | 72 | Chi Kit | Ng | Constraining gravitational wave amplitude birefringence with GWTC-3 | ||||||||||||||||||||||
75 | 73 | Shania | Nichols | Exploring the Origins of Loud Glitches in aLIGO Detector Data | ||||||||||||||||||||||
76 | 74 | Swadha | Pandey | Axion Dark-Matter Birefringent Cavity (ADBC) | ||||||||||||||||||||||
77 | 75 | Lucia | Papalini | Exploring Deep Learning Techniques to enable Early Warning for Compact Binary Coalescences | ||||||||||||||||||||||
78 | 76 | Jason | Poon | Gravitational Wave Lensing Lens Reconstruction | ||||||||||||||||||||||
79 | 77 | Giada | Caneva Santoro | First constraints on compact binary environments from LIGO-Virgo data | ||||||||||||||||||||||
80 | 78 | Eungwang | Seo | Gravitational lensing aided luminosity distance estimation for compact binary coalescences | ||||||||||||||||||||||
81 | 79 | Minori | Shikauchi | Triggered GW Searches by sGRB Afterglow Observations with the CHIME telescope | ||||||||||||||||||||||
82 | 80 | Kaido | Suzuki | Development of a signal amplification technique with nonlinear optical effects for next-generation gravitational wave detectors | ||||||||||||||||||||||
83 | 81 | Satoru | Takano | The Cryogenic Monolithic Interferometer for TOrsion-Bar Antenna | ||||||||||||||||||||||
84 | 82 | Kyouhei | Takatani | Comparison of noise reduction performance using auxiliary channels between CNN and LSTM | ||||||||||||||||||||||
85 | 83 | Kotaro | Takeguchi | Development of a diamagnetic levitation system for a macroscopic quantum measurement | ||||||||||||||||||||||
86 | 84 | Masahide | Tamaki | Calculation of heat flow in KAGRA cryogenic payload | ||||||||||||||||||||||
87 | 85 | Daiki | Tanabe | Study of bulk deformation and rotation of ETM caused by Photon Calibrator | ||||||||||||||||||||||
88 | 86 | Kota | Tomita | Toward machine learning analysis of gravitational wave time series and signal detection | ||||||||||||||||||||||
89 | 87 | Darkhan | Tuyenbayev | Development of SEISA - a Software System for Accessing Instrument Data | ||||||||||||||||||||||
90 | 88 | Masaki | Uematsu | Searching origin of binary black hole with gravitational wave observation | ||||||||||||||||||||||
91 | 89 | Laura | Uronen | Under the lens: Casting light on black hole mergers | ||||||||||||||||||||||
92 | 90 | Federico | De Santi | Gravitational Waves from Binary Close Encounters: Fast Parameter Estimation with Normalizing Flows | ||||||||||||||||||||||
93 | 91 | Michele | Vacatello | Glitches classification in Advanced Virgo O3 with machine learning | ||||||||||||||||||||||
94 | 92 | Jasper | Venneberg | Bright Squeezed Light Generation and Quantum Correlation Measurements | ||||||||||||||||||||||
95 | 93 | Sophie | Bini | Search for hyperbolic encounters of compact objects in the third LIGO-Virgo-KAGRA observing run | ||||||||||||||||||||||
96 | 94 | Verónica | Villa-Ortega | Detectability of thermal effects in binary neutron-star post mergers | ||||||||||||||||||||||
97 | 95 | He | Wang | Intelligent Noise Suppression for Gravitational Wave Observational Data | ||||||||||||||||||||||
98 | 96 | Zi-Yu | Wang | GNS, current and furture | ||||||||||||||||||||||
99 | 97 | Daiki | Watarai | Physically consistent gravitational waveform for capturing beyond general relativity effects in the compact object merger phase | ||||||||||||||||||||||
100 | 98 | Yumeng | Xu | Role of non-linear memory in breaking the distance-inclination angle degeneracy for ground based gravitational waves detectors |