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Jan 27, 2025360Brew: A Decoder-only Foundation Model for Personalized Ranking and RecommendationJan 24, 2025Humanity's Last ExamJan 15, 2025Chemically-Disordered Transparent Conductive Perovskites with High Crystalline FidelityJan 14, 2025Realization of a doped quantum antiferromagnet with dipolar tunnelings in a Rydberg tweezer arrayJan 14, 2025Roadmap on Neuromorphic PhotonicsJan 6, 2025The fragmentation of molecular clouds in starburst environmentsJan 2, 2025FEASTS: Radial Distribution of HI surface densities down to 0.01 M$_{\odot}$ pc$^{-2}$ of 35 Nearby GalaxiesDec 23, 2024A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO surveyDec 19, 2024Data for Mathematical Copilots: Better Ways of Presenting Proofs for Machine LearningDec 18, 2024Measurement of the branching fraction and $\it CP$-violating asymmetry of the decay $B^{0} \rightarrow π^{0} π^{0}$ using $387$ million bottom-antibottom meson pairs in Belle II dataDec 18, 2024The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interactionDec 12, 2024Two Earth-size Planets and an Earth-size Candidate Transiting the Nearby Star HD 101581Nov 22, 2024The NANOGrav 15 Yr Data Set: Removing Pulsars One by One from the Pulsar Timing ArrayNov 20, 2024The NANOGrav 15 yr Data Set: Harmonic Analysis of the Pulsar Angular CorrelationsNov 18, 2024Fault-tolerant quantum computation with a neutral atom processorNov 14, 2024Artificial Intelligence for Quantum ComputingNov 5, 2024MuCol Milestone Report No. 5: Preliminary ParametersNov 4, 2024The JCMT BISTRO Survey: The Magnetic Fields of the IC 348 Star-forming RegionOct 28, 2024CaloChallenge 2022: A Community Challenge for Fast Calorimeter SimulationOct 7, 2024A-SLOTH reveals the nature of the first stars