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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Prof. Niranjan Thatte

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Instrumentation
  • Exoplanets and planetary physics

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Exoplanets and Stellar Physics
  • Galaxy formation and evolution
  • Extremely Large Telescope
Niranjan.Thatte@physics.ox.ac.uk
Telephone: 01865 (2)73412
Denys Wilkinson Building, room 709
  • About
  • Teaching
  • Publications

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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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.
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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
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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
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Analysis and mitigation of pupil discontinuities on adaptive optics performance

SPIE, the international society for optics and photonics 10703 (2018) 1070322

Authors:

Noah Schwartz, Jean-François Sauvage, Carlos Correia, Benoit Neichel, Thierry Fusco, Fernando Quiros-Pacheco, Kjetil Dohlen, Kacem El Hadi, Guido Agapito, Niranjan Thatte, Fraser Clarke
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