A dataset provided by the European Space Agency

Name 12181
Title The Atmospheric Structure of Giant Hot Exoplanets
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12181;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-sl28q8b
Author Deming, Drake
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12181&mission=hst
Publication
  • ACCESS: a featureless optical transmission spectrum for WASP-19b from Magellan/IMACS
  • A Consistent Retrieval Analysis of 10 Hot Jupiters Observed in Transmission
  • A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion
  • A large range of haziness conditions in hot-Jupiter atmospheres
  • A Near-infrared Transmission Spectrum for the Warm Saturn HAT-P-12b
  • A New Approach to Analyzing HST Spatial Scans: The Transmission Spectrum of HD 209458 b
  • A new method to correct for host star variability in multiepoch observations of exoplanet transmission spectra
  • An HST optical-to-near-IR transmission spectrum of the hot Jupiter WASP-19b: detection of atmospheric water and likely absence of TiO
  • A Population Study of Gaseous Exoplanets
  • A re-analysis of equilibrium chemistry in five hot Jupiters
  • Assessing the C/O Ratio Formation Diagnostic: A Potential Trend with Companion Mass
  • Atmospheric Characterization of Five Hot Jupiters with the Wide Field Camera 3 on the Hubble Space Telescope
  • Atmospheric Characterization of Hot Jupiter CoRoT-1 b Using the Wide Field Camera 3 on the Hubble Space Telescope
  • Broadband transmission spectroscopy of HD 209458b with ESPRESSO: evidence for Na, TiO, or both
  • Cloud Atlas: Hubble Space Telescope Near-infrared Spectral Library of Brown Dwarfs, Planetary-mass Companions, and Hot Jupiters
  • Detection of a westward hotspot offset in the atmosphere of hot gas giant CoRoT-2b
  • ExoGAN: Retrieving Exoplanetary Atmospheres Using Deep Convolutional Generative Adversarial Networks
  • Exoplanet Transit Spectroscopy of Hot Jupiters Using HST/WFC3
  • Exoplanet Transit Spectroscopy Using WFC3: WASP-12 b, WASP-17 b, and WASP-19 b
  • Exploring the Ability of Hubble Space Telescope WFC3 G141 to Uncover Trends in Populations of Exoplanet Atmospheres through a Homogeneous Transmission Survey of 70 Gaseous Planets
  • Five Key Exoplanet Questions Answered via the Analysis of 25 Hot-Jupiter Atmospheres in Eclipse
  • HD 209458b in new light: evidence of nitrogen chemistry, patchy clouds and sub-solar water
  • H2O abundances and cloud properties in ten hot giant exoplanets
  • H2O Abundances in the Atmospheres of Three Hot Jupiters
  • Impact of Planetary Mass Uncertainties on Exoplanet Atmospheric Retrievals
  • Infrared Transmission Spectroscopy of the Exoplanets HD 209458b and XO-1b Using the Wide Field Camera-3 on the Hubble Space Telescope
  • Marginalizing Instrument Systematics in HST WFC3 Transit Light Curves
  • Methods for Incorporating Model Uncertainty into Exoplanet Atmospheric Analysis
  • On the synergy between Ariel and ground-based high-resolution spectroscopy
  • Optical to Near-infrared Transmission Spectrum of the Warm Sub-Saturn HAT-P-12b
  • Optical Transmission Spectra of Hot Jupiters: Effects of Scattering
  • Physical properties and optical-infrared transmission spectrum of the giant planet XO-1 b
  • Probing the extreme planetary atmosphere of WASP-12b
  • Retrieval analysis of 38 WFC3 transmission spectra and resolution of the normalization degeneracy
  • Retrieval of planetary and stellar properties in transmission spectroscopy with AURA
  • Signatures of Nitrogen Chemistry in Hot Jupiter Atmospheres
  • Statistical Analysis of Hubble/WFC3 Transit Spectroscopy of Extrasolar Planets
  • The Emergent 1.1-1.7 mm Spectrum of the Exoplanet CoRoT-2b as Measured Using the Hubble Space Telescope
  • The Importance of Optical Wavelength Data on Atmospheric Retrievals of Exoplanet Transmission Spectra
  • The Precision of Mass Measurements Required for Robust Atmospheric Characterization of Transiting Exoplanets
  • The PYRAT BAY framework for exoplanet atmospheric modelling: a population study of Hubble/WFC3 transmission spectra
  • Unveiling cloudy exoplanets: the influence of cloud model choices on retrieval solutions
  • Wayne--A Simulator for HST WFC3 IR Grism Spectroscopy
Instrument WFC3, WFC3/IR
Temporal Coverage 2010-09-08T02:17:05Z/2012-09-25T21:27:45Z
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 2013-09-26T17:18:06Z
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, Deming comma Drake, 2013, 'The Atmospheric Structure of Giant Hot Exoplanets', 1.0, European Space Agency, https://doi.org/10.5270/esa-sl28q8b