ELT HARMONI: image slicer preliminary design

Proceedings of SPIE: Ground-based and Airborne Instrumentation for Astronomy VII Society of Photo-Optical Instrumentation Engineers 10702 (2018)

Authors:

F Laurent, D Boudon, J Kosmalski, M Loupias, G Raffault, A Remillieux, Niranjan Thatte, I Bryson, H Schnetler, F Clarke, Matthias Tecza

Abstract:

Harmoni is the ELT's first light visible and near-infrared integral field spectrograph. It will provide four different spatial scales, ranging from coarse spaxels of 60 × 30 mas best suited for seeing limited observations, to 4 mas spaxels that Nyquist sample the diffraction limited point spread function of the ELT at near-infrared wavelengths. Each spaxel scale may be combined with eleven spectral settings, that provide a range of spectral resolving powers from R 3500 to R 20000 and instantaneous wavelength coverage spanning the 0.47 - 2.45 μm wavelength range of the instrument. The consortium consists of several institutes in Europe under leadership of Oxford University. Harmoni is starting its Final Design Phase after a Preliminary Design Phase in November, 2017. The CRAL has the responsibility of the Integral Field Unit design linking the Preoptics to the 4 Spectrographs. It is composed of a field splitter associated with a relay system and an image slicer that create from a rectangular Field of View a very long (540mm) output slit for each spectrograph. In this paper, the preliminary design and performances of Harmoni Image Slicer will be presented including image quality, pupil distortion and slit geometry. It has been designed by CRAL for Harmoni PDR in November, 2017. Special emphases will be put on straylight analysis and slice diffraction. The optimisation of the manufacturing and slit geometry will also be reported.

HARMONI pre-optics design at PDR

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

Authors:

MA Cagigas, E Hernandez, JL Rasilla, E Mediavilla, B García-Lorenzo, JM Herreros, JV Gigante, LF Rodriguez, I Bryson, M Schnedtler, F Clarke, M Tecza, N Thatte

MICHI: a thermal-infrared instrument for the TMT

SPIE, the international society for optics and photonics 10702 (2018) 10702a0

Authors:

Chris Packham, Mitsuhiko Honda, Mark Chun, Itsuki Sakon, Matthew Richter, Yoshiko Okamoto, Hirokazu Kataza, Christian Marois, Michael Meyer, Manoj Puravankara, Jayne Birkby, Ian Crossfield, Thayne Curry, Thomas Greathouse, Gregory Herczeg, Kohei Ichikawa, Hanae Inami, Masatoshi Imanishi, Enrique Lopez-Rodriguez

The HARMONI/ELT spectrographs

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

Authors:

Myriam Arnal Rodrigues, John Capone, Andrew Earle, Tom Foster, A Hidalgo, I Lewis, J Lynn, K O'brien, I Tosh, EM George, M Accardo, D Alvarez, R Conzelmann, J Hopgood, F Clarke, H Schnetler, M Tecza, N Thatte

MOSAIC: the ELT Multi-Object Spectrograph

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

Authors:

P Jagourel, E Fitzsimons, F Hammer, F de Frondat Laadim, M Puech, CJ Evans, I Guinouard, F Chemla, M Frotin, Y Yang, P Parr-Burman, T Morris, M Dubbeldam, M Close, K Middleton, G Rousset, E Gendron, A Kelz, A Janssen, J Pragt, R Navarro, M Larrieu, K El Hadi, K Dohlen

Abstract:

Following a successful Phase A study, we introduce the delivered conceptual design of the MOSAIC1 multi-object spectrograph for the ESO Extremely Large Telescope (ELT). MOSAIC will provide R~5000 spectroscopy over the full 460-1800 nm range, with three additional high-resolution bands (R~15000) targeting features of particular interest. MOSAIC will combine three operational modes, enabling integrated-light observations of up to 200 sources on the sky (high-multiplex mode) or spectroscopy of 10 spatially-extended fields via deployable integral-field units: MOAO6 assisted high-definition (HDM) and Visible IFUs (VIFU). We will summarise key features of the sub-systems of the design, e.g. the smart tiled focal-plane for target selection and the multi-object adaptive optics used to correct for atmospheric turbulence, and present the next steps toward the construction phase.