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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
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Teaching Insights

Education

School is to make students 'Yearn to Learn'. College is to get students to 'Learn to Learn'

Laser Tomographic AO system for an integral field spectrograph on the E-ELT: ATLAS project

AO for ELT 2011 - 2nd International Conference on Adaptive Optics for Extremely Large Telescopes (2011)

Authors:

T Fusco, S Meimon, Y Clénet, M Cohen, H Schnetler, J Paufique, V Michau, N Thatte, N Hubin, C Petit, JP Amans, D Gratadour, JM Conan, P Jagourel

Abstract:

ATLAS is a generic Laser Tomographic AO (LTAO) system for the E-ELT. Based on modular, relatively simple, and yet innovative concepts, it aims at providing diffraction-limited images in the near infra-red for a close to 100 percent sky coverage.

Testing the limit of AO for ELTs: Diffraction limited astronomy in the red optical

AO for ELT 2011 - 2nd International Conference on Adaptive Optics for Extremely Large Telescopes (2011)

Authors:

M Tecza, J Magorrian, N Thatte, F Clarke

Abstract:

Many of the proposed science cases for extremely large telescopes (ELT) are only possible because of the unprecedented sensitivity and spatial resolution due to advanced, e.g. tomographic and multi conjugate, adaptive optic (AO) systems. Current AO systems on 8-10 m telescopes work best at wavelengths longward of 1 μm with Strehl ratios ≥ 15%. At red-optical wavelengths, e.g. in the I band (0.8 μm), the Strehl ratio is at best a few percent. The AO point spread function (PSF) typically has a diffraction-limited core superimposed on the seeing halo, however, for a 5% Strehl ratio the core has a very low intensity above the seeing halo. At an ELT, due to a 3-4 times higher angular resolution, the diffraction limited PSF core of only 5% Strehl ratio stands more prominently atop the shallow seeing halo leading to almost diffraction limited image quality even at low Strehl ratios. Prominent ELT science cases that use the Calcium triplet can exploit this gain in spatial resolution in the red-optical: stellar populations in dense environments or crowded fields; and the case of intermediate mass black holes in nuclear and globular stellar clusters, as well as (super-) massive black holes in galaxies.

SWIFT observations of the Arp 147 ring galaxy system

Monthly Notices of the Royal Astronomical Society (2011)

Authors:

L Fogarty, N Thatte, M Tecza, F Clarke, T Goodsall, R Houghton, G Salter, RL Davies, SA Kassin

The Gemini NICI Planet-Finding Campaign: Discovery of a substellar L dwarf companion to the nearby young M dwarf CD-35 2722

Astrophysical Journal Letters 729:2 (2011)

Authors:

Z Wahhaj, MC Liu, BA Biller, F Clarke, EL Nielsen, LM Close, T Hayward, EE Mamajek, M Cushing, T Dupuy
More details from the publisher
More details
Details from ArXiV

An image slicer-based integral-field spectrograph for EPICS

Proceedings of SPIE - The International Society for Optical Engineering 7735:PART 1 (2010)

Authors:

M Tecza, N Thatte, G Salter, F Clarke

Abstract:

We present the results of a design study for an integral field spectrograph as the "back-end" instrument for spectroscopy of exoplanets carried out in the context of the EPICS Phase A study. EPICS is the planet finder imager and spectrograph for the E-ELT. In our study we investigated the feasibility of an image slicer based integral field spectrograph and developed an optical design for the image slicer and the necessary pre-optics, as well as the spectrograph optics. We present a detailed analysis of the optical performance of the design. © 2010 Copyright SPIE - The International Society for Optical Engineering.
More details from the publisher

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