Showing 721–740 of 5,527 results
/ Date/ Name
Apr 27, 2024Spin-dependent $π$$π^{\ast}$ gap in graphene on a magnetic substrateApr 26, 2024Constraints On Covariant WIMP-Nucleon Effective Field Theory Interactions from the First Science Run of the LUX-ZEPLIN ExperimentApr 24, 2024Observational Parameters of Blue Large-amplitude PulsatorsApr 23, 2024JWST detections of amorphous and crystalline HDO ice toward massive protostarsApr 22, 2024Study of $e^+e^-\toωX(3872)$ and $γX(3872)$ from 4.66 to 4.95 GeVApr 21, 2024The PEPSI Exoplanet Transit Survey (PETS). V: New Na D transmission spectra indicate a quieter atmosphere on HD 189733bApr 19, 2024Determination of the CKM angle $φ_{3}$ from a combination of Belle and Belle II resultsApr 16, 2024First double-differential cross section measurement of neutral-current $π^0$ production in neutrino-argon scattering in the MicroBooNE detectorApr 16, 2024New AGN diagnostic diagrams based on the [OIII]$λ4363$ auroral lineApr 16, 2024Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometryApr 16, 2024A 25-micron single photon sensitive kinetic inductance detectorApr 15, 2024Deep JWST/NIRCam imaging of Supernova 1987AApr 15, 2024First search for light fermionic dark matter absorption on electrons using germanium detector in CDEX-10 experimentApr 15, 2024Using Micromegas detectors for direct dark matter searches: challenges and perspectivesApr 14, 2024PDRs4All IX. Sulfur elemental abundance in the Orion BarApr 12, 2024Absolute dimensions of solar-type eclipsing binaries. NY Hya: A test for magnetic stellar evolution modelsApr 12, 2024Development of a data overflow protection system for Super-Kamiokande to maximize data from nearby supernovaeApr 12, 2024Technical Design Report of the Spin Physics Detector at NICAApr 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, 2024Quiescent or dusty? Unveiling the nature of extremely red galaxies at $z>3$