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The Hubble diagram of type Ia supernovae as a function of host galaxy morphology
Affiliation:Department of Physics, University of Durham, South Road, Durham DH1 3LE;California Institute of Technology, E. California Blvd, Pasadena, CA 91125, USA;E. O. Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA;Department of Physics, Stockholm University, SCFAB, S-106 91 Stockholm, Sweden;LPNHE, CNRS-IN2P3, University of Paris VI &VII, Paris, France;Colorado College, 14 East Cache La Poudre Street, Colorado Springs, CO 80903, USA;Department of Physics, University of California Berkeley, Berkeley, CA 94720-7300, USA;American Astronomical Society, 2000 Florida Ave, NW, Suite 400, Washington, DC 20009, USA;Department of Astronomy and Research Centre for the Early Universe, School of Science, University of Tokyo, Tokyo 113-0033, Japan;IST, Lisbon, Portugal;Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA;Department of Physics, University of Oxford, Nuclear &Astrophysics Laboratory, Keble Road, Oxford OX1 3RH;Institute of Astronomy, Madingley Road, Cambridge CB3 0HA;Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37240, USA;European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19, Chile;Department of Astronomy, University of Barcelona, Barcelona, Spain;Isaac Newton Group of Telescopes, Apartado de Correos 321, E-38700 Santa Cruz de La Palma, Islas Canarias, Spain;University of Texas, Department of Astronomy, C-1400, Austin, TX 78712, USA;National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan
Abstract:
Keywords:supernovae: general    cosmological parameters    cosmology: observations    distance scale
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