Showing 541–560 of 6,168 results
/ Date/ Name
Nov 29, 2024A New Look at Disk Winds and External Photoevaporation in the $σ$-Orionis ClusterNov 28, 2024Towards a new generation of solid total-energy detectors for neutron-capture time-of-flight experiments with intense neutron beamsNov 27, 2024X-ray and gamma-ray timing of GRB 180720B, GRB 181222B, GRB 211211A and GRB 220910A observed with Fermi and ASIMNov 22, 2024The NANOGrav 15 Yr Data Set: Removing Pulsars One by One from the Pulsar Timing ArrayNov 21, 2024An accurate solar axions ray-tracing response of BabyIAXONov 21, 2024Exact and approximate error bounds for physics-informed neural networksNov 20, 2024The NANOGrav 15 yr Data Set: Harmonic Analysis of the Pulsar Angular CorrelationsNov 20, 2024EWOCS-III: JWST observations of the supermassive star cluster Westerlund 1Nov 19, 2024The GAPS Programme at TNG. LXV. Precise density measurement of TOI-1430 b, a young planet with an evaporating atmosphereNov 18, 2024Miscentering of Optical Galaxy Clusters Based on Sunyaev-Zeldovich CounterpartsNov 18, 2024DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering MeasurementsNov 18, 2024DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and QuasarsNov 18, 2024DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering StatisticsNov 18, 2024Fault-tolerant quantum computation with a neutral atom processorNov 15, 2024Large quadrupole deformation in $^{20}$Ne challenges rotor model and modern theory: urging for $α$ clusters in nucleiNov 15, 2024The Fate of the Interstellar Medium in Early-type Galaxies. V. AGN Feedback from Optical Spectral ClassificationNov 15, 2024BICEP/Keck XIX: Extremely Thin Composite Polymer Vacuum Windows for BICEP and Other High Throughput Millimeter Wave TelescopesNov 9, 2024Integrated-Photonics-Based Systems for Polarization-Gradient Cooling of Trapped IonsNov 8, 2024Magnetic structure and crystal field states of antiferromagnetic CeNiGe$_3$: Neutron scattering and $μ$SR investigationsNov 8, 2024A simple model for spectroscopic analyses of active stars