An integrated payload design for the Exoplanet Characterisation Observatory (EChO)

Bruce Swinyard; Giovanna Tinetti; Jonathan Tennyson; Marcell Tessenyi; Ingo Waldmann; Bruce Swinyard; Paul Eccleston; Marc Ferlet; Tanya Lim; Alberto Adriani; Giuseppe Piccioni; Jean-Philippe Beaulieu; Tomas Belenguer Davila; Gonzalo Ramos Zapata; Neil Bowles; Ian Bryson; Gillian Wright; Athena Coustenis; Vincent Coudé Du Foresto; Jean-Michel Reess; Paul Hartogh; Pierre-Olivier Lagage; Giuseppe Malaguti; Gianluca Morgante; Mercedes López-Morales; Ignasi Ribas; Giuseppina Micela; Hans Ulrik Nørgaard-Nielsen; Marc Ollivier; Emanuele Pace; Enzo Pascale; Alessandro Sozzetti; Mark R. Swain; Berend Winter; Maria-Rosa Zapatero Osorio

doi:10.1117/12.924688

An integrated payload design for the Exoplanet Characterisation Observatory (EChO)

Bruce Swinyard, Giovanna Tinetti, Jonathan Tennyson, Marcell Tessenyi, Ingo Waldmann, Bruce Swinyard, Paul Eccleston, Marc Ferlet, Tanya Lim, Alberto Adriani, Giuseppe Piccioni, Jean-Philippe Beaulieu, Tomas Belenguer Davila, Gonzalo Ramos Zapata, Neil Bowles, Ian Bryson, Gillian Wright, Athena Coustenis, Vincent Coudé Du Foresto, Jean-Michel ReessPaul Hartogh, Pierre-Olivier Lagage, Giuseppe Malaguti, Gianluca Morgante, Mercedes López-Morales, Ignasi Ribas, Giuseppina Micela, Hans Ulrik Nørgaard-Nielsen, Marc Ollivier, Emanuele Pace, Enzo Pascale, Alessandro Sozzetti, Mark R. Swain, Berend Winter, Maria-Rosa Zapatero Osorio

National Space Institute

Research output: Contribution to journal › Conference article › Research › peer-review

Abstract

The Exoplanet Characterisation Observatory (EChO) is a space mission dedicated to undertaking spectroscopy of transiting exoplanets over the widest wavelength range possible. It is based around a highly stable space platform with a 1.2 m class telescope. The mission is currently being studied by ESA in the context of a medium class mission within the Cosmic Vision programme for launch post 2020. The payload suite is required to provide simultaneous coverage from the visible to the mid-infrared and must be highly stable and effectively operate as a single instrument. In this paper we describe the integrated spectrometer payload design for EChO which will cover the 0.4 to 16 micron wavelength band. The instrumentation is subdivided into 5 channels (Visible/Near Infrared, Short Wave InfraRed, 2 x Mid Wave InfraRed; Long Wave InfraRed) with a common set of optics spectrally dividing the input beam via dichroics. We discuss the significant design issues for the payload and the detailed technical trade-offs that we are undertaking to produce a payload for EChO that can be built within the mission and programme constraints and yet which will meet the exacting scientific performance required to undertake transit spectroscopy. © 2012 SPIE.

Original language	English
Journal	Proceedings of SPIE, the International Society for Optical Engineering
Volume	8442
Pages (from-to)	84421G
Number of pages	14
ISSN	0277-786X
DOIs	https://doi.org/10.1117/12.924688
Publication status	Published - 2012
Event	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray - Amsterdam RAI Convention Ctr., Amsterdam, Netherlands Duration: 1 Jul 2012 → 6 Jul 2012 Conference number: 8443

Conference

Conference	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Number	8443
Location	Amsterdam RAI Convention Ctr.
Country/Territory	Netherlands
City	Amsterdam
Period	01/07/2012 → 06/07/2012

Keywords

Astronomy
Buildings
Design
Infrared radiation
Millimeter waves
Observatories
Space flight
Space platforms
Space telescopes
Spectrometers
Instruments

Access to Document

10.1117/12.924688

Cite this

Swinyard, B., Tinetti, G., Tennyson, J., Tessenyi, M., Waldmann, I., Swinyard, B., Eccleston, P., Ferlet, M., Lim, T., Adriani, A., Piccioni, G., Beaulieu, J-P., Davila, T. B., Zapata, G. R., Bowles, N., Bryson, I., Wright, G., Coustenis, A., Du Foresto, V. C., ... Osorio, M-R. Z. (2012). An integrated payload design for the Exoplanet Characterisation Observatory (EChO). Proceedings of SPIE, the International Society for Optical Engineering, 8442, 84421G. https://doi.org/10.1117/12.924688

Swinyard, Bruce ; Tinetti, Giovanna ; Tennyson, Jonathan ; Tessenyi, Marcell ; Waldmann, Ingo ; Swinyard, Bruce ; Eccleston, Paul ; Ferlet, Marc ; Lim, Tanya ; Adriani, Alberto ; Piccioni, Giuseppe ; Beaulieu, Jean-Philippe ; Davila, Tomas Belenguer ; Zapata, Gonzalo Ramos ; Bowles, Neil ; Bryson, Ian ; Wright, Gillian ; Coustenis, Athena ; Du Foresto, Vincent Coudé ; Reess, Jean-Michel ; Hartogh, Paul ; Lagage, Pierre-Olivier ; Malaguti, Giuseppe ; Morgante, Gianluca ; López-Morales, Mercedes ; Ribas, Ignasi ; Micela, Giuseppina ; Nørgaard-Nielsen, Hans Ulrik ; Ollivier, Marc ; Pace, Emanuele ; Pascale, Enzo ; Sozzetti, Alessandro ; Swain, Mark R. ; Winter, Berend ; Osorio, Maria-Rosa Zapatero. / An integrated payload design for the Exoplanet Characterisation Observatory (EChO). In: Proceedings of SPIE, the International Society for Optical Engineering. 2012 ; Vol. 8442. pp. 84421G.

@inproceedings{c74076f5e4144b11ba4fa7b339128267,

title = "An integrated payload design for the Exoplanet Characterisation Observatory (EChO)",

abstract = "The Exoplanet Characterisation Observatory (EChO) is a space mission dedicated to undertaking spectroscopy of transiting exoplanets over the widest wavelength range possible. It is based around a highly stable space platform with a 1.2 m class telescope. The mission is currently being studied by ESA in the context of a medium class mission within the Cosmic Vision programme for launch post 2020. The payload suite is required to provide simultaneous coverage from the visible to the mid-infrared and must be highly stable and effectively operate as a single instrument. In this paper we describe the integrated spectrometer payload design for EChO which will cover the 0.4 to 16 micron wavelength band. The instrumentation is subdivided into 5 channels (Visible/Near Infrared, Short Wave InfraRed, 2 x Mid Wave InfraRed; Long Wave InfraRed) with a common set of optics spectrally dividing the input beam via dichroics. We discuss the significant design issues for the payload and the detailed technical trade-offs that we are undertaking to produce a payload for EChO that can be built within the mission and programme constraints and yet which will meet the exacting scientific performance required to undertake transit spectroscopy. {\textcopyright} 2012 SPIE.",

keywords = "Astronomy, Buildings, Design, Infrared radiation, Millimeter waves, Observatories, Space flight, Space platforms, Space telescopes, Spectrometers, Instruments",

author = "Bruce Swinyard and Giovanna Tinetti and Jonathan Tennyson and Marcell Tessenyi and Ingo Waldmann and Bruce Swinyard and Paul Eccleston and Marc Ferlet and Tanya Lim and Alberto Adriani and Giuseppe Piccioni and Jean-Philippe Beaulieu and Davila, {Tomas Belenguer} and Zapata, {Gonzalo Ramos} and Neil Bowles and Ian Bryson and Gillian Wright and Athena Coustenis and {Du Foresto}, {Vincent Coud{\'e}} and Jean-Michel Reess and Paul Hartogh and Pierre-Olivier Lagage and Giuseppe Malaguti and Gianluca Morgante and Mercedes L{\'o}pez-Morales and Ignasi Ribas and Giuseppina Micela and N{\o}rgaard-Nielsen, {Hans Ulrik} and Marc Ollivier and Emanuele Pace and Enzo Pascale and Alessandro Sozzetti and Swain, {Mark R.} and Berend Winter and Osorio, {Maria-Rosa Zapatero}",

year = "2012",

doi = "10.1117/12.924688",

language = "English",

volume = "8442",

pages = "84421G",

journal = "Proceedings of SPIE, the International Society for Optical Engineering",

issn = "0277-786X",

publisher = "S P I E - International Society for Optical Engineering",

note = "Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray ; Conference date: 01-07-2012 Through 06-07-2012",

}

Swinyard, B, Tinetti, G, Tennyson, J, Tessenyi, M, Waldmann, I, Swinyard, B, Eccleston, P, Ferlet, M, Lim, T, Adriani, A, Piccioni, G, Beaulieu, J-P, Davila, TB, Zapata, GR, Bowles, N, Bryson, I, Wright, G, Coustenis, A, Du Foresto, VC, Reess, J-M, Hartogh, P, Lagage, P-O, Malaguti, G, Morgante, G, López-Morales, M, Ribas, I, Micela, G, Nørgaard-Nielsen, HU, Ollivier, M, Pace, E, Pascale, E, Sozzetti, A, Swain, MR, Winter, B & Osorio, M-RZ 2012, 'An integrated payload design for the Exoplanet Characterisation Observatory (EChO)', Proceedings of SPIE, the International Society for Optical Engineering, vol. 8442, pp. 84421G. https://doi.org/10.1117/12.924688

An integrated payload design for the Exoplanet Characterisation Observatory (EChO). / Swinyard, Bruce; Tinetti, Giovanna; Tennyson, Jonathan; Tessenyi, Marcell; Waldmann, Ingo; Swinyard, Bruce; Eccleston, Paul; Ferlet, Marc; Lim, Tanya; Adriani, Alberto; Piccioni, Giuseppe; Beaulieu, Jean-Philippe; Davila, Tomas Belenguer; Zapata, Gonzalo Ramos; Bowles, Neil; Bryson, Ian; Wright, Gillian; Coustenis, Athena; Du Foresto, Vincent Coudé; Reess, Jean-Michel; Hartogh, Paul; Lagage, Pierre-Olivier; Malaguti, Giuseppe; Morgante, Gianluca; López-Morales, Mercedes; Ribas, Ignasi; Micela, Giuseppina; Nørgaard-Nielsen, Hans Ulrik; Ollivier, Marc; Pace, Emanuele; Pascale, Enzo; Sozzetti, Alessandro; Swain, Mark R.; Winter, Berend; Osorio, Maria-Rosa Zapatero.

In: Proceedings of SPIE, the International Society for Optical Engineering, Vol. 8442, 2012, p. 84421G.

Research output: Contribution to journal › Conference article › Research › peer-review

TY - GEN

T1 - An integrated payload design for the Exoplanet Characterisation Observatory (EChO)

AU - Swinyard, Bruce

AU - Tinetti, Giovanna

AU - Tennyson, Jonathan

AU - Tessenyi, Marcell

AU - Waldmann, Ingo

AU - Swinyard, Bruce

AU - Eccleston, Paul

AU - Ferlet, Marc

AU - Lim, Tanya

AU - Adriani, Alberto

AU - Piccioni, Giuseppe

AU - Beaulieu, Jean-Philippe

AU - Davila, Tomas Belenguer

AU - Zapata, Gonzalo Ramos

AU - Bowles, Neil

AU - Bryson, Ian

AU - Wright, Gillian

AU - Coustenis, Athena

AU - Du Foresto, Vincent Coudé

AU - Reess, Jean-Michel

AU - Hartogh, Paul

AU - Lagage, Pierre-Olivier

AU - Malaguti, Giuseppe

AU - Morgante, Gianluca

AU - López-Morales, Mercedes

AU - Ribas, Ignasi

AU - Micela, Giuseppina

AU - Nørgaard-Nielsen, Hans Ulrik

AU - Ollivier, Marc

AU - Pace, Emanuele

AU - Pascale, Enzo

AU - Sozzetti, Alessandro

AU - Swain, Mark R.

AU - Winter, Berend

AU - Osorio, Maria-Rosa Zapatero

N1 - Conference code: 8443

PY - 2012

Y1 - 2012

N2 - The Exoplanet Characterisation Observatory (EChO) is a space mission dedicated to undertaking spectroscopy of transiting exoplanets over the widest wavelength range possible. It is based around a highly stable space platform with a 1.2 m class telescope. The mission is currently being studied by ESA in the context of a medium class mission within the Cosmic Vision programme for launch post 2020. The payload suite is required to provide simultaneous coverage from the visible to the mid-infrared and must be highly stable and effectively operate as a single instrument. In this paper we describe the integrated spectrometer payload design for EChO which will cover the 0.4 to 16 micron wavelength band. The instrumentation is subdivided into 5 channels (Visible/Near Infrared, Short Wave InfraRed, 2 x Mid Wave InfraRed; Long Wave InfraRed) with a common set of optics spectrally dividing the input beam via dichroics. We discuss the significant design issues for the payload and the detailed technical trade-offs that we are undertaking to produce a payload for EChO that can be built within the mission and programme constraints and yet which will meet the exacting scientific performance required to undertake transit spectroscopy. © 2012 SPIE.

AB - The Exoplanet Characterisation Observatory (EChO) is a space mission dedicated to undertaking spectroscopy of transiting exoplanets over the widest wavelength range possible. It is based around a highly stable space platform with a 1.2 m class telescope. The mission is currently being studied by ESA in the context of a medium class mission within the Cosmic Vision programme for launch post 2020. The payload suite is required to provide simultaneous coverage from the visible to the mid-infrared and must be highly stable and effectively operate as a single instrument. In this paper we describe the integrated spectrometer payload design for EChO which will cover the 0.4 to 16 micron wavelength band. The instrumentation is subdivided into 5 channels (Visible/Near Infrared, Short Wave InfraRed, 2 x Mid Wave InfraRed; Long Wave InfraRed) with a common set of optics spectrally dividing the input beam via dichroics. We discuss the significant design issues for the payload and the detailed technical trade-offs that we are undertaking to produce a payload for EChO that can be built within the mission and programme constraints and yet which will meet the exacting scientific performance required to undertake transit spectroscopy. © 2012 SPIE.

KW - Astronomy

KW - Buildings

KW - Design

KW - Infrared radiation

KW - Millimeter waves

KW - Observatories

KW - Space flight

KW - Space platforms

KW - Space telescopes

KW - Spectrometers

KW - Instruments

U2 - 10.1117/12.924688

DO - 10.1117/12.924688

M3 - Conference article

VL - 8442

SP - 84421G

JO - Proceedings of SPIE, the International Society for Optical Engineering

JF - Proceedings of SPIE, the International Society for Optical Engineering

SN - 0277-786X

T2 - Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray

Y2 - 1 July 2012 through 6 July 2012

ER -

An integrated payload design for the Exoplanet Characterisation Observatory (EChO)

Abstract

Conference

Keywords

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