Showing 1–19 of 19 results
/ Date/ Name
Dec 6, 2025A XRISM/Resolve view of the dynamics in the hot gaseous atmosphere of M87Oct 28, 2025XRISM/Resolve reveals the complex iron structure of NGC 7213: Evidence for radial stratification between inner disk and broad-line regionMay 28, 2020Measurement of jet-medium interactions via direct photon-hadron correlations in Au$+$Au and $d$$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVMay 10, 2018Beam-energy and centrality dependence of direct-photon emission from ultra-relativistic heavy-ion collisionsMar 5, 2018Measurement of two-particle correlations with respect to second- and third-order event planes in Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVFeb 3, 2017Measurements of $e^+e^-$ pairs from open heavy flavor in $p$+$p$ and $d$+$A$ collisions at $\sqrt{s_{NN}}=200$ GeVFeb 28, 2015Detailed Shape and Evolutionary Behavior of the X-ray Luminosity Function of Active Galactic NucleiMay 16, 2013A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveysNov 10, 2010Electronic structure of an antiferromagnetic metal: CaCrO3Dec 6, 2007Field dependence of the quantum ground state in the Shastry-Sutherland system SrCu$_2$(BO$_3$)$_2$Oct 29, 2007NMR evidence for the persistence of spin-superlattice above the 1/8 magnetization plateau in SrCu2(BO3)2Mar 16, 2007The XMM-Newton serendipitous survey IV. The AXIS X-ray source counts and angular clusteringNov 30, 2006Observation Campaign of SS 433 in April 2006Oct 10, 2006Muon-spin relaxation measurements on the dimerized spin-1/2 chains NaTiSi2O6 and TiOClApr 21, 2004Field-Induced Effects of Anisotropic Magnetic Interactions in SrCu2(BO3)2Jul 18, 2001A Possible Emission Feature in an X-ray Afterglow of GRB970828 as a Radiative Recombination EdgeMay 2, 2000Soundwave Anomalies in SrCu_{2}(BO_{3})_{2}Jan 11, 2000Magnetic Susceptibilities of Spin-1/2 Antiferromagnetic Heisenberg Ladders and Applications to Ladder Oxide CompoundsJan 18, 1998Optical Identification of the Hardest X-ray Source in the ASCA Large Sky Survey