List of posters

The links to the PDF of the posters are highlighted in red.

 

Comparative planetology in the Solar System

  • 1.1 Investigating the scattered light from planetary atmospheres with polarimetry: Esther Buenzli − ETH Zurich, Switzerland
  • 1.2 A multidisciplinary investigation of Martian atmospheric chemistry: Maria Duffy − The Open University, UK
  • 1.3 The Chemical Composition of Simulated Titan's Mid-Atmospheric Aerosols: Diana Laufer − Tel Aviv University, Israel
  • 1.4 Seeing Double at Neptune's South Pole: Statia Luszcz-Cook − U.C. Berkeley, USA
  • 1.5 Cyclostrophic wind in Venus mesosphere from the Venus Express temperature retrievals: Arianna Piccialli − Max Planck Institute for Solar System Research, Germany
  • 1.6 Global GCM simulations of Jupiter's atmosphere: Roland Young − University of Oxford, UK
  • 1.7 An analysis of Pluto occultation light curves using an atmospheric radiative- conductive model: troposphere case: Angela Zalucha − Massachusetts Institute of Technology, USA

    • Giant exoplanets

  • 2.1 The atmospheres and orbital eccentricities of WASP planets: David Anderson − Keele University, UK
  • 2.2 3D hydrodynamical simulations of substellar objects' atmospheres: Veronica Arias − Hamburger Sternwarte, Germany
  • 2.3 Within the Atmosphere of WASP-14b: Jasmina Blecic − University of Central Florida, USA
  • 2.4 The Orbit of WASP-12b: Christopher Campo − University of Central Florida, USA
  • 2.5 Characterizing Planetary Atmospheres with Narrow-Band Transit Photometry: Knicole Colón − University of Florida, USA
  • 2.6 Characterization of the extrasolar planet TrES-1b: Patricio Cubillos − University of Central Florida, USA
  • 2.7 The effect of scattering clouds and dust on extrasolar planet emission spectra: Remco de Kok − SRON Netherlands Institute for Space Research, Netherlands
  • 2.8 Optical and near-infrared measurements of dayside-emission from hot Jupiters: Ernst de Mooij − Leiden Observatory, Netherlands
  • 2.9 Ultraviolet transmission spectroscopy of the transiting exoplanet WASP-12b: Luca Fossati − The Open University, UK
  • 2.10 A new look at NICMOS transmission spectroscopy: Neale Gibson − University of Oxford, UK
  • 2.11 Secondary Eclipse Phase Measurements from the Spitzer ToO Program: Ryan Hardy − University of Central Florida, USA
  • 2.12 Retrieval of Exoplanet Atmospheric Structure and Composition from Transit Spectroscopy: Lee Jaemin − AOPP/Oxford, UK
  • 2.13 A Ground-Based Optical Transmission Spectrum Survey of the Atmospheres of Transiting Exoplanets: Line Analysis and Future Work: Adam Jensen − Wesleyan University, USA
  • 2.14 Three-dimensional atmospheric circulation of hot Jupiters on highly eccentric orbits: Tiffany Kataria − University of Arizona, LPL, USA
  • 2.15 Spitzer lightcurves of the ultrashort period, massive hot Jupiter WASP-18b: Pierre Maxted − Keele University, UK
  • 2.16 Two Multi-Wavelength Secondary Eclipses of WASP-18b: Sarah Nymeyer − University of Central Florida, USA
  • 2.17 Hot Jupiters in a tube and Hyperdog for planetary sniffing: Robert Peale − University of Central Florida, USA
  • 2.18 On the radius of hot Jupiters: Frédéric Pont − University of Exeter, UK
  • 2.19 A Ground-Based Optical Transmission Spectrum Survey of the Atmospheres of Transiting Exoplanets: First Results: Seth Redfield − Wesleyan University, USA
  • 2.20 Ground-based Photometric Detections of Thermal Emission from hot Jupiters: Justin Rogers − Johns Hopkins University, USA
  • 2.21 Spectral comparison of directly imaged, young substellar companions using integral field spectroscopy; construction of an empiric log g sequence: Tobias Schmidt − Astrophysical Institute Jena, Germany
  • 2.22 Spectral and Polarimetric characterization of gaseous and telluric planets with SEE COAST: Jean Schneider − Paris Observatory, France
  • 2.23 Transmission spectroscopy of the sodium doublet in WASP-17b with VLT: Patricia Wood − Keele University, UK
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    Terrestrial exoplanets

  • 3.1 The spectro-photometric variability of the globally-integrated infrared emission of terrestrial planets: Illeana Gomez − Laboratoire d'Astrophysique de Bordeaux, France
  • 3.2 Spectropolarimetric signals of Earth-like exoplanets with clouds: Theodora Karalidi − SRON-Netherlands Institute for Space Research, Netherlands
  • 3.3 Influence of clouds in atmospheres of Earth-like extrasolar planets: Daniel Kitzmann − Technische Universität Berlin, Germany
  • 3.4 An Energy-balance model for tidally-heated ocean planets: Alastair McKinstry − National University of Ireland, Ireland
  • 3.5 Reflectance spectra of irradiated Earth-like exoplanets: Mariana Wagner − Sternwarte Hamburg, Germany
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    Bridging the gap

  • 4.1 Extra-solar planetary interior and atmospheric structure models: Victoria Bending − The Open University, UK
  • 4.2 Some Crucial Aspects of Exoplanet Atmosphere Dynamics Modeling: James Cho − Queen Mary, University of London, UK
  • 4.3 Planetary Polar Vortices: Instabilities in Nature and in the Laboratory: Luca Montabone − LMD-Universite Paris VI / AOPP-University of Oxford, France / UK
  • 4.4 The impact of microphysics on optical properties of shallow cumulus clouds based on Large Eddy Simulations. The EULAG model and its ability to simulate exoplanets: Joanna Sławińska − Institute of Geophysics, University of Warsaw, Poland
  • 4.5 Planetary Atmospheric Circulation Regimes in a Simplified GCM: Yixiong Wang - University of Oxford, UK
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    Living planets

  • 5.1 Earth Glint Observations Conducted During the Deep Impact Spacecraft Flyby: Richard Barry − NASA Laboratory for Exoplanets and Stellar Astrophysics, USA
  • 5.2 Influence of the stellar spectral flux distribution on surface habitability and atmospheric dynamics of Earth-like extrasolar planets: Mareike Godolt − Zentrum für Astronomie und Astrophysik, TU Berlin
  • 5.3 Response of ozone photochemical pathways to a doubling in CO2: Mareike Godolt − Zentrum für Astronomie und Astrophysik, TU Berlin
  • 5.4 Simulating Earth as an Extrasolar Planet: Tyler Robinson − University of Washington, USA
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