Showing 41–60 of 66 results
/ Date/ Name
Sep 27, 2022Report of the Topical Group on Physics Beyond the Standard Model at Energy Frontier for Snowmass 2021Jul 28, 2022An Insight-HXMT view of the mHz quasi-regular modulation phenomenon in the black hole X-ray binary 4U 1630-47Mar 21, 2022An Adaptive Optics Census of Companions to Northern Stars Within 25 pc with Robo-AOAug 10, 2021End-to-End User Behavior Retrieval in Click-Through RatePrediction ModelMay 27, 2021Large Adaptive Optics Survey for Substellar Objects (LASSO) Around Young, Nearby, Low-mass Stars with Robo-AOMay 6, 2021An Ultrahigh-Q Microresonator on 4H-silicon-carbide-on-insulator Platform for Multiple Harmonics, Cascaded Raman Lasing and Kerr Comb GenerationsMar 8, 2021InFillmore: Frame-Guided Language Generation with Bidirectional ContextJan 10, 2021Towards Long-term Fairness in RecommendationOct 19, 2020Strain-mediated high conductivity in ultrathin antiferromagnetic metallic nitridesJul 11, 2019Privileged Features Distillation at Taobao RecommendationsApr 15, 2019Personalized Re-ranking for RecommendationApr 14, 2019BERT4Rec: Sequential Recommendation with Bidirectional Encoder Representations from TransformerFeb 3, 2019Value-aware Recommendation based on Reinforced Profit Maximization in E-commerce SystemsNov 5, 2018Identifying the Best Machine Learning Algorithms for Brain Tumor Segmentation, Progression Assessment, and Overall Survival Prediction in the BRATS ChallengeAug 8, 2018Signatures of long-range-correlated disorder in the magnetotransport of ultrathin topological insulatorsJul 13, 2018LASSO: Large Adaptive optics Survey for Substellar Objects using the new SAPHIRA detector on Robo-AOJul 12, 2018Velocity-resolved reverberation mapping of five bright Seyfert 1 galaxiesApr 20, 2017Space Telescope and Optical Reverberation Mapping Project. VII. Understanding the UV anomaly in NGC 5548 with X-Ray SpectroscopyOct 28, 2014Characterization of the LIGO detectors during their sixth science runOct 22, 2014Searching for stochastic gravitational waves using data from the two co-located LIGO Hanford detectors