Showing 1–20 of 97 results
/ Date/ Name
Feb 25, 1999Decoherence and Programmable Quantum ComputationDec 22, 1999Automatic Quantum Error CorrectionDec 2, 2020The SEDIGISM survey: first data release and overview of the Galactic structureMar 4, 2022The SEDIGISM survey: Molecular cloud morphology. I. Classification and star formationNov 28, 2007Determining the relative evolutionary stages of very young massive star formation regionsOct 12, 2021The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky WayMay 4, 2022The SEDIGISM survey: Molecular cloud morphology. II. Integrated source propertiesNov 21, 2021The SEDIGISM survey: a search for molecular outflowsMay 12, 2023Large-scale Velocity-coherent Filaments in the SEDIGISM Survey: Association with Spiral Arms and Fraction of Dense GasSep 28, 2009The effects of superconductor-stabilizer interfacial resistance on quench of current-carrying coated conductorAug 15, 2017The power of the AC-DC circuit: Operating principles of a simple multi-functional transcriptional network motifSep 13, 2005The Integration of YBCO Coated Conductors into Magnets and Rotating MachineryDec 23, 2005A CH3CN and HCO+ survey towards southern methanol masers associated with star formationOct 12, 2004AC Loss in Striped (Filamentary) YBCO Coated Conductors Leading to Designs for High Frequencies and Field-Sweep AmplitudesApr 13, 2017Quantum error correction failure distributions: comparison of coherent and stochastic error modelsDec 24, 2016HCN hyperfine ratio analysis of massive molecular clumpsOct 4, 2001Measurement of the 3He mass diffusion coefficient in superfluid 4He over the 0.45-0.95 K temperature rangeSep 22, 2015Scaling properties of fractional momentum loss of high-pT hadrons in nucleus-nucleus collisions at $\sqrt{s_{_{NN}}}$ from 62.4 GeV to 2.76 TeVOct 9, 2014Beam-energy and system-size dependence of the space-time extent of the pion emission source produced in heavy ion collisionsApr 8, 2014Measurement of $Υ$(1S+2S+3S) production in $p$$+$$p$ and Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeV