Showing 61–80 of 242 results
/ Date/ Name
Oct 10, 2024Spectropolarimetry of SN 2023ixf reveals both circumstellar material and helium core to be asphericalSep 19, 2024RAD-Bench: Evaluating Large Language Models Capabilities in Retrieval Augmented DialoguesSep 17, 2024SLAck: Semantic, Location, and Appearance Aware Open-Vocabulary TrackingAug 19, 2024RV measurements of directly imaged brown dwarf GQ Lup B to search for exo-satellitesAug 19, 2024Fringing analysis and forward modeling of Keck Planet Imager and Characterizer (KPIC) spectraAug 15, 2024One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating ProgenitorsJul 30, 2024Atmospheric characterization of the super-Jupiter HIP 99770 b with KPICJul 1, 2024Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle II experimentJun 28, 2024CSAKD: Knowledge Distillation with Cross Self-Attention for Hyperspectral and Multispectral Image FusionJun 28, 2024Enhancing Stability for Large Language Models Training in Constrained Bandwidth NetworksJun 17, 2024Using graph neural networks to reconstruct charged pion showers in the CMS High Granularity CalorimeterMay 31, 2024SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 $μ$m and Data Release for the COSMOS FieldMay 30, 2024Search for the decay $B^{0}\toγγ$ using Belle and Belle II dataMay 23, 2024Let's Fuse Step by Step: A Generative Fusion Decoding Algorithm with LLMs for Robust and Instruction-Aware ASR and OCRMay 12, 2024Search for lepton-flavor-violating $τ^- \to μ^-μ^+μ^-$ decays at Belle IIMay 6, 2024Physical properties and electronic structure of the two-gap superconductor V$_{2}$Ga$_{5}$Apr 19, 2024Determination of the CKM angle $φ_{3}$ from a combination of Belle and Belle II resultsApr 16, 2024The Ninth NTIRE 2024 Efficient Super-Resolution Challenge ReportApr 15, 2024NTIRE 2024 Challenge on Image Super-Resolution ($\times$4): Methods and ResultsApr 11, 2024Orbital and Atmospheric Characterization of the 1RXS J034231.8+121622 System Using High-Resolution Spectroscopy Confirms That The Companion is a Low-Mass Star