Showing 21–40 of 50 results
/ Date/ Name
Nov 17, 2016VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMANov 12, 2016The Herschel-ATLAS: a sample of 500μm-selected lensed galaxies over 600 square degreesAug 31, 2015Cold Dust Emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: Dependence on Luminosity, Obscuration & AGN ActivityMar 30, 2015Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMAMar 3, 2015A multi-wavelength exploration of the [CII]/IR ratio in H-ATLAS/GAMA galaxies out to z=0.2May 4, 2014In situ electromagnetic field diagnostics with an electron plasma in a Penning-Malmberg trapNov 11, 2013An ALMA survey of sub-millimeter galaxies in the Extended Chandra Deep Field South: Sub-millimeter properties of color-selected galaxiesJun 7, 2012The JCMT Nearby Galaxies Legacy Survey VIII. CO data and the L(CO3-2)-L(FIR) correlation in the SINGS sampleJan 18, 2012Antihydrogen and mirror-trapped antiproton discrimination: Discriminating between antihydrogen and mirror-trapped antiprotons in a minimum-B trapJul 14, 2011Gas and dust in a submillimeter galaxy at z = 4.24 from the Herschel ATLASApr 26, 2011Centrifugal separation and equilibration dynamics in an electron-antiproton plasmaApr 24, 2011Alpha Antihydrogen ExperimentMar 16, 2011GAMA/H-ATLAS: The ultraviolet spectral slope and obscuration in galaxiesNov 4, 2010The Detection of a Population of Submillimeter-Bright, Strongly-Lensed GalaxiesJul 20, 2010The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIREMar 16, 2010Molecular and Atomic Gas in the Local Group Galaxy M33Feb 16, 2010Antihydrogen formation dynamics in a multipolar neutral anti-atom trapJul 1, 2008A novel antiproton radial diagnostic based on octupole induced ballistic lossJun 30, 2008Compression of Antiproton Clouds for Antihydrogen TrappingMay 27, 2008Particle Physics Aspects of Antihydrogen Studies with ALPHA at CERN