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Rendering of ELT instruments on ELT Nasmyth Platform (credit ESO/L. Calçada)

Rendering of ELT instruments on ELT Nasmyth Platform

Credit: credit ESO/L. Calçada

Dr Fraser Clarke

Senior Programme Manager for Space Instrumentation

Research theme

  • Instrumentation
  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Space instrumentation
fraser.clarke@physics.ox.ac.uk
  • About
  • Publications

Near infrared throughput and stray light measurements of diffraction gratings for ELT-HARMONI

Proceedings of SPIE Society of Photo-optical Instrumentation Engineers 10706 (2018)

Authors:

M Rodrigues, John Capone, F Clarke, A Earle, T Foster, J Lynn, K Obrien, M Tecza, NA Thatte, I Tosh, A Hidalgo Valadez, IJ Lewis
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Sensing and control of segmented mirrors with a pyramid wavefront sensor in the presence of spiders

(2018)

Authors:

Noah Schwartz, Jean-François Sauvage, Carlos Correia, Cyril Petit, Fernando Quiros-Pacheco, Thierry Fusco, Kjetil Dohlen, Kacem El Hadi, Niranjan Thatte, Fraser Clarke, Jérome Paufique, Joel Vernet
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ELT HARMONI: Image Slicer Preliminary Design

(2018)

Authors:

Florence Laurent, Didier Boudon, Johan Kosmalski, Magali Loupias, Guillaume Raffault, Alban Remillieux, Niranjan Thatte, Ian Bryson, Hermine Schnetler, Fraser Clarke, Matthias Tecza
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Opto-mechanical designs for the HARMONI adaptive optics systems

Proceedings of SPIE SPIE 10703 (2018)

Authors:

K Dohlen, TJ Morris, J Piqueras Lopez, A Calcines-Rosario, A Costille, M Dubbeldam, K El Hadi, T Fusco, M Llored, B Neichel, S Pascal, J-F Sauvage, P Vola, Fraser Clarke, H Schnetler, I Bryson, Niranjan Thatte

Abstract:

HARMONI is a visible and near-infrared integral field spectrograph equipped with two complementary adaptive optics systems, fully integrated within the instrument. A Single Conjugate AO (SCAO) system offers high performance for a limited sky coverage and a Laser Tomographic AO (LTAO) system provides AO correction with a very high sky-coverage. While the deformable mirror performing real-time correction of the atmospheric disturbances is located within the telescope itself, the instrument contains a suite of state-of-the-art and innovative wavefront sensor systems. Laser guide star sensors (LGSS) are located at the entrance of the instrument and fed by a dichroic beam splitter, while the various natural guide star sensors for LTAO and SCAO are located close to the science focal plane. We present opto-mechanical architecture and design at PDR level for these wavefront sensor systems.
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System analysis and expected performance of a high-contrast module for HARMONI

SPIE, the international society for optics and photonics 10702 (2018) 107029n

Authors:

Alexis Carlotti, François Hénault, Kjetil Dohlen, Jean-François Sauvage, Patrick Rabou, Yves Magnard, Arthur Vigan, David Mouillet, Gael Chauvin, Pascal Vola, Mickael Bonnefoy, Thierry Fusco, Kacem El Hadi, Niranjan Thatte, Fraser Clarke, Matthias Tecza, Ian Bryson, Hermine Schnetler, Christophe Vérinaud
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