Showing 21–40 of 43 results
/ Date/ Name
Apr 6, 2016The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance IndicatorsMar 11, 2016The Carnegie Chicago Hubble Program: The Mid-Infrared Colours of Cepheids and the Effect of Metallicity on the CO Band-head at $4.6μ$mDec 18, 2015Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 2: The Physics Program for DUNE at LBNFFeb 24, 2015The Carnegie Hubble Program: The Distance and Structure of the SMC as Revealed by Mid-infrared Observations of CepheidsJan 2, 2015A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)Sep 24, 2014A New Cepheid Distance Measurement and Method for NGC 6822Aug 8, 2014Improving Photoelectron Counting and Particle Identification in Scintillation Detectors with Bayesian TechniquesJul 28, 2014The Calibration of the WISE W1 and W2 Tully-Fisher RelationJun 24, 2013The Carnegie Hubble Program: The Infrared Leavitt Law in IC 1613Apr 22, 2013The impact of bars on disk breaks as probed by S4G imagingJan 21, 2013Calibration of the Mid-Infrared Tully-Fisher RelationSep 22, 2012The Carnegie Hubble Program: The Leavitt Law at 3.6 and 4.5 micron in the Milky WayAug 16, 2012Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble ConstantOct 27, 2011The 2010 Interim Report of the Long-Baseline Neutrino Experiment Collaboration Physics Working GroupsAug 23, 2011The Carnegie Hubble Program: The Leavitt Law at 3.6 μm and 4.5 μm in the Large Magellanic CloudMar 16, 2011GAMA/H-ATLAS: The ultraviolet spectral slope and obscuration in galaxiesNov 4, 2010The Detection of a Population of Submillimeter-Bright, Strongly-Lensed GalaxiesSep 3, 2010Galaxy and Mass Assembly (GAMA): survey diagnostics and core data releaseAug 4, 2010Mid-Infrared Galaxy Morphology from the Spitzer Survey of Stellar Structure in Galaxies (S^4G): The Imprint of the de Vaucouleurs Revised Hubble-Sandage Classification System at 3.6 micronsApr 20, 2010The UV-Optical Color Dependence of Galaxy Clustering in the Local Universe