Showing 21–40 of 1,145 results
/ Date/ Name
Mar 31, 2026The SPHEREx Instrument: Calibration, testing and performance measurements of the NIR 2 spectroscopic surveyor from the laboratory to in-orbit commissioningMar 26, 2026Voxtral TTSMar 20, 2026Coma Physics of an Interstellar Object: JWST Spatial-Spectral Mapping of 3I/ATLASMar 5, 2026Early Planet Formation in Embedded Disks (eDisk). XVIII. Indication of a possible spiral structure in the dust-continuum emission of the protostellar disk around IRAS 16544-1604 in CB 68Mar 3, 2026Accretion onto the Embedded Protostar L1527 IRS: Insights from JWST NIRSpec and MIRI ObservationsMar 2, 2026The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): Constraints on disk turbulence, fragmentation velocity, and inner pebble fluxesFeb 27, 2026Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScienceFeb 24, 2026A Path to an All-Sky Survey with RomanFeb 24, 2026ALMA Central Molecular Zone Exploration Survey (ACES)-IV. Data of the two intermediate-width spectral windowsFeb 23, 2026ALMA Central molecular zone Exploration Survey (ACES) VI: ALMA Large Program Reveals a Highly Filamentary Central Molecular ZoneFeb 23, 2026A Very Big Video Reasoning SuiteFeb 21, 2026Chat-Based Support Alone May Not Be Enough: Comparing Conversational and Embedded LLM Feedback for Mathematical Proof LearningFeb 19, 2026Building an AI-native Research Ecosystem for Experimental Particle Physics: A Community VisionFeb 19, 2026Computer-Using World ModelFeb 11, 2026Evidence for Shallow Nebular Attenuation Curves and Patchy Dust Geometry at z~2 with Pa-beta/H-alpha Measurements from JWST-MegaScience Medium Band PhotometryFeb 11, 2026Voxtral RealtimeFeb 10, 2026Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 using JWST and ALMAFeb 5, 2026Multi-Token Prediction via Self-DistillationFeb 3, 2026Ferroelectric dynamic-field-driven nucleation and growth model for predictive materials-to-circuit co-designFeb 2, 2026Pilots and Other Predictable Elements of the Starlink Ku-Band Downlink