Showing 1–20 of 30 results
/ Date/ Name
Mar 26, 2018OH as an Alternate Tracer for Molecular Gas: Excitation Temperatures of the OH 18-cm Main Lines in W5Feb 2, 2015The Structure of Dark Molecular Gas in the Galaxy - I: A Pilot Survey for 18-cm OH Emission Towards $l \approx 105^°, b \approx +1^°$Oct 2, 2013Pierre Auger Observatory and Telescope Array: Joint Contributions to the 33rd International Cosmic Ray Conference (ICRC 2013)Jun 20, 2013Project X: Physics OpportunitiesFeb 20, 2012Faint Extended OH Emission from the Local Interstellar Medium in the Direction l \approx 108\circ, b \approx 5\circJan 13, 2012Radio & Optical Interferometry: Basic Observing Techniques and Data AnalysisNov 28, 2011The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger ObservatoryJul 24, 2011The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related MeasurementsJul 24, 2011The Pierre Auger Observatory III: Other Astrophysical ObservationsApr 2, 2011Five supernova survey galaxies in the southern hemisphere. II. The supernova ratesJan 24, 2011Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger ObservatoryMar 13, 2009Mass Transport Processes and their Roles in the Formation, Structure, and Evolution of Stars and Stellar SystemsMar 5, 2009Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger ObservatoryAug 4, 2008The volume densities of giant molecular clouds in M83May 29, 2008Crowded-Field Astrometry with SIM PlanetQuest. II. An Improved Instrument ModelJul 2, 2007Station-Keeping Requirements for Constellations of Free-Flying Collectors Used for Astronomical Imaging in SpaceApr 2, 2007A Comparison between Anomalous 6-cm H$_2$CO Absorption and CO(1-0) Emission in the L1204/S140Jul 27, 2006Anomalous H_2CO Absorption Towards the Galactic Anticenter: A Blind Search for Dense Molecular CloudsMay 24, 2006NGC922 - A new drop-through ring galaxyNov 24, 2004The Opacity of Spiral Galaxy Disks IV: Radial Extinction Profiles from Counts of Distant Galaxies seen through Foreground Disks