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Design and performance of the Exo-planet Characterisation Observatory (EChO) integrated payload

  • Bruce Swinyard
  • , Marcel Tessenyi
  • , Giovanna Tinetti
  • , Ingo Waldmann
  • , Paul Eccleston
  • , Marc Ferlet
  • , Ranah Irshad
  • , Tanya Lim
  • , Kevin Middleton
  • , Tom Bradshaw
  • , Martin Crook
  • , Tom Hunt
  • , Berend Winter
  • , Ian Bryson
  • , Naidu Bezawada
  • , William Taylor
  • , Neil Bowles
  • , Enzo Pascale
  • , Gianluca Morgante
  • , Emanuele Pace
  • Alberto Adriani, Jean Michel Reess, Pierre Drossart, Vincent Coudé Du Foresto, Marc Ollivier, Roland Ottensamer, Mirek Rataj, Gonzalo Ramos Zapata, Jan Rutger Schrader, Avri Selig, Kate Isaak, Martin Linder, Ludovic Puig, Paul Hartogh, Christophe Lovis, Giusi Micela, Ignasi Ribas, Ignas Snellen, Jean Phillippe Beaulieu
  • UCL University College London
  • STFC Rutherford Appleton Laboratory
  • Department of Physics and Astronomy
  • University College London
  • Royal Observatory
  • University of Oxford
  • Cardiff Law School
  • INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna
  • University of Florence
  • Osservatorio Astrofisico di Torino
  • UPMC University Paris 06
  • Institut d’Astrophysique Spatiale
  • University of Vienna
  • Space Research Centre of the Polish Academy of Sciences (CBK PAN)
  • Carretera de Ajalvir
  • SRON-Netherlands Institute for Space Research
  • ESTEC - European Space Research and Technology Centre
  • Max-Planck-Institut für Sonnensystemforschung
  • University of Geneva
  • INAF - Osservatorio Astronomico di Palermo
  • Universitat Autònoma de Barcelona 
  • Instituut Lorentz for Theoretical Physics
  • Institut d 'Astrophysique de Paris

Research output: Chapter in Book/Report/Conference proceedingConference paperpeer-review

2 Citations (Scopus)

Abstract

The Exoplanet Characterisation Observatory (EChO) mission was one of the proposed candidates for the European Space Agency's third medium mission within the Cosmic Vision Framework. EChO was designed to observe the spectra from transiting exoplanets in the 0.55-11 micron band with a goal of covering from 0.4 to 16 microns. The mission and its associated scientific instrument has now undergone a rigorous technical evaluation phase and we report here on the outcome of that study phase, update the design status and review the expected performance of the integrated payload and satellite.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation 2014
Subtitle of host publicationOptical, Infrared, and Millimeter Wave
EditorsJacobus M. Oschmann, Mark Clampin, Howard A. MacEwen, Giovanni G. Fazio
PublisherSPIE
ISBN (Electronic)9780819496119
DOIs
Publication statusPublished - 2014
EventSpace Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave - Montreal, Canada
Duration: 22 Jun 201427 Jun 2014

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume9143
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceSpace Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Country/TerritoryCanada
CityMontreal
Period22/06/201427/06/2014

Keywords

  • Astronomy
  • Exoplanets
  • Space missions
  • Spectrometers

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