Showing 681–700 of 6,913 results
/ Date/ Name
Oct 21, 2024UVCANDELS: Catalogs of photometric redshifts and galaxy physical propertiesOct 21, 2024A Novel high-z submm Galaxy Efficient Line Survey in ALMA bands 3 through 8 -- An ANGELS PilotOct 21, 2024Programmable entangled qubit states on a linear-optical platformOct 18, 2024First results from the JWST Early Release Science Program Q3D: The Fast Outflow in a Red Quasar at z=0.44Oct 17, 2024Sliding Puzzles Gym: A Scalable Benchmark for State Representation in Visual Reinforcement LearningOct 17, 2024Observation of $χ_{c0}\toΣ^{+}\barΣ^{-}η$ and evidence for $χ_{c1,2}\toΣ^{+}\barΣ^{-}η$Oct 17, 2024Observation of the Singly Cabibbo-Suppressed Decay $Λ_c^{+}\to pπ^0$Oct 17, 2024Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASOOct 15, 2024Null models for comparing information decomposition across complex systemsOct 14, 2024Seven wonders of Cosmic Dawn: JWST confirms a high abundance of galaxies and AGNs at z $\simeq$ 9-11 in the GLASS fieldOct 14, 2024Spectroscopic confirmation of a dust-obscured, metal-rich dwarf galaxy at z~5Oct 14, 2024Incommensurate Transverse Peierls TransitionOct 14, 2024Shining Light on the Dark Sector: Search for Axion-like Particles and Other New Physics in Photonic Final States with FASEROct 14, 2024Measurement of the double-differential cross section of muon-neutrino charged-current interactions with low hadronic energy in the NOvA Near DetectorOct 11, 2024Observation of $D^+\toη^\primeμ^+ν_μ$ and First Study of $D^+\to η^\prime \ell^+ν_\ell$ Decay DynamicsOct 10, 2024Spectropolarimetry of SN 2023ixf reveals both circumstellar material and helium core to be asphericalOct 9, 2024First Very Long Baseline Interferometry Detections at 870μmOct 9, 2024Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their HostsOct 9, 2024Observation of disorder-free localization using a (2+1)D lattice gauge theory on a quantum processorOct 7, 2024Polycyclic Aromatic Hydrocarbon and CO(2-1) Emission at 50-150 pc Scales in 70 Nearby Galaxies