Showing 81–100 of 249 results
/ Date/ Name
Jun 21, 2024Pistis-RAG: Enhancing Retrieval-Augmented Generation with Human FeedbackJun 14, 2024SEACrowd: A Multilingual Multimodal Data Hub and Benchmark Suite for Southeast Asian LanguagesJun 8, 2024The PLATO MissionJun 4, 2024The computational power of random quantum circuits in arbitrary geometriesApr 23, 2024JWST detections of amorphous and crystalline HDO ice toward massive protostarsApr 22, 2024Squeezing the quantum noise of a gravitational-wave detector below the standard quantum limitApr 16, 2024The Ninth NTIRE 2024 Efficient Super-Resolution Challenge ReportApr 11, 2024Birds of a Feather: Resolving Stellar Mass Assembly With JWST/NIRCam in a Pair of Kindred $z \sim 2$ Dusty Star-forming Galaxies Lensed by the PLCK G165.7+67.0 ClusterApr 11, 2024A broad linewidth, compact, millimeter-bright molecular emission line source near the Galactic CenterApr 10, 2024JWST/MIRI detection of suprathermal OH rotational emissions: probing the dissociation of the water by Lyman alpha photons near the protostar HOPS 370Apr 4, 2024The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy FieldsMar 18, 2024Decoding Compressed Trust: Scrutinizing the Trustworthiness of Efficient LLMs Under CompressionFeb 16, 2024TimeSeriesBench: An Industrial-Grade Benchmark for Time Series Anomaly Detection ModelsFeb 6, 2024JWST observations of $^{13}$CO$_{2}$ ice: Tracing the chemical environment and thermal history of ices in protostellar envelopesFeb 5, 2024Revisiting VAE for Unsupervised Time Series Anomaly Detection: A Frequency PerspectiveJan 29, 2024MIRI MRS Observations of Beta Pictoris I. The Inner Dust, the Planet, and the GasDec 18, 2023JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at $z=0.4$Dec 13, 2023IPA: Class 0 Protostars Viewed in CO Emission Using JWSTDec 6, 2023The Initial Mass Function Based on the Full-sky 20-pc Census of $\sim$3,600 Stars and Brown DwarfsNov 30, 2023Evaluating the feasibility of short-integration scans based on the 2022 VGOS-R&D program