A dataset provided by the European Space Agency

Name 9447
Title Characterizing the Atmosphere of an Extrasolar Planet
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9447;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-iy1rxfe
Author Charbonneau, David
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9447&mission=hst
Publication
  • A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion
  • A large range of haziness conditions in hot-Jupiter atmospheres
  • A limit on the presence of Earth-mass planets around a Sun-like star
  • A re-analysis of equilibrium chemistry in five hot Jupiters
  • A SEA BASS on the Exoplanet HD 209458b
  • Broadband transmission spectroscopy of HD 209458b with ESPRESSO: evidence for Na, TiO, or both
  • Detecting new planets in transiting systems
  • Determining Atmospheric Conditions at the Terminator of the Hot Jupiter HD 209458b
  • Effect of the Eccentricity of the Planets Orbit on the Limb Darkening Coefficients of the Eclipsed Star
  • Ground-based detection of sodium in the transmission spectrum of exoplanet HD 209458b
  • HD 209458b in new light: evidence of nitrogen chemistry, patchy clouds and sub-solar water
  • Homogeneous studies of transiting extrasolar planets - I. Light-curve analyses
  • H2O abundances and cloud properties in ten hot giant exoplanets
  • Hubble Space Telescope STIS Optical Transit Transmission Spectra of the Hot Jupiter HD 209458b
  • Identification of Absorption Features in an Extrasolar Planet Atmosphere
  • Infrared Transmission Spectroscopy of the Exoplanets HD 209458b and XO-1b Using the Wide Field Camera-3 on the Hubble Space Telescope
  • Is there Na I in the atmosphere of HD 209458b?. Effect of the centre-to-limb variation and Rossiter-McLaughlin effect in transmission spectroscopy studies
  • Limb darkening laws for two exoplanet host stars derived from 3D stellar model atmospheres. Comparison with 1D models and HST light curve observations
  • Methods for Incorporating Model Uncertainty into Exoplanet Atmospheric Analysis
  • MOST Space-based Photometry of the Transiting Exoplanet System HD 209458: Transit Timing to Search for Additional Planets
  • On stellar limb darkening and exoplanetary transits
  • Retrieving the transmission spectrum of HD 209458b using CHOCOLATE: a new chromatic Doppler tomography technique
  • The Importance of Optical Wavelength Data on Atmospheric Retrievals of Exoplanet Transmission Spectra
  • The signature of hot hydrogen in the atmosphere of the extrasolar planet HD 209458b
  • The upper atmosphere of the exoplanet HD 209458 b revealed by the sodium D lines. Temperature-pressure profile, ionization layer, and thermosphere
  • The Very Low Albedo of an Extrasolar Planet: MOST Space-based Photometry of HD 209458
  • TiO and VO broad band absorption features in the optical spectrum of the atmosphere of the hot-Jupiter HD 209458b
  • Using Stellar Limb-Darkening to Refine the Properties of HD 209458b
Instrument STIS/CCD
Temporal Coverage 2003-05-03T11:48:01Z/2003-07-06T05:32:27Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2004-07-08T18:25:45Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Charbonneau comma David, 2004, 'Characterizing the Atmosphere of an Extrasolar Planet', 1.0, European Space Agency, https://doi.org/10.5270/esa-iy1rxfe