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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.

Matthias Tecza

HARMONI Instrument Scientist

Research theme

  • Astronomy and astrophysics
  • Instrumentation

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Exoplanet atmospheres
  • Exoplanets and Stellar Physics
  • Extremely Large Telescope
matthias.tecza@physics.ox.ac.uk
Telephone: 01865 (2)73364
Denys Wilkinson Building, room 361G
  • About
  • Teaching
  • Publications

Simulating the detection and classification of high-redshift supernovae with HARMONI on the ELT

Monthly Notices of the Royal Astronomical Society Oxford University Press 478:3 (2018) 3189-3198

Authors:

S Bounissou, Niranjan Thatte, S Zieleniewski, RCW Houghton, M Tecza, I Hook, B Neichel, T Fusco

Abstract:

We present detailed simulations of integral field spectroscopic observations of a supernova in a host galaxy at z ∼ 3, as observed by the HARMONI spectrograph on the Extremely Large Telescope, asssisted by laser tomographic adaptive optics. The goal of the simulations, using the HSIM simulation tool, is to determine whether HARMONI can discern the supernova Type from spectral features in the supernova spectrum. We find that in a 3 hour observation, covering the near-infrared H and K bands, at a spectral resolving power of ∼3000, and using the 20×20 mas spaxel scale, we can classify supernova Type Ia and their redshift robustly up to 80 days past maximum light (20 days in the supernova rest frame). We show that HARMONI will provide spectra at z ∼ 3 that are of comparable (or better) quality to the best spectra we can currently obtain at z ∼ 1, thus allowing studies of cosmic expansion rates to be pushed to substantially higher redshifts.
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CASTAway: An asteroid main belt tour and survey.

Advances in Space Research Elsevier 62:8 (2017) 1998-2025

Authors:

Neil E Bowles, C Snodgrass, JP Sanchez, Jessica A Arnold, P Eccleston, T Andert, A Probst, G Naletto, AC Vandaele, de de Leon, A Nathues, IR Thomas, N Thomas, L Jorda, V da Deppo, H Haack, SF Green, B Carry, Kerri L Donaldson Hanna, J Leif Jorgensen, A Kereszturi, FE DeMeo, JK Davies, Fraser Clarke, K Kinch, A Guilbert-Lepoutre, J Agarwal, AS Rivkin, P Pravec, S Fornasier, M Gravnik, RH Jones, N Murdoch, KH Joy, Matthias Tecza, Jennifer M Barnes, J Licandro, BT Greenhagen, Simon B Calcutt, Charlotte M Marriner, Tristram J Warren, I Tosh

Abstract:

CASTAway is a mission concept to explore our Solar System’s main asteroid belt. Asteroids and comets provide a window into the formation and evolution of our Solar System and the composition of these objects can be inferred from space-based remote sensing using spectroscopic techniques. Variations in composition across the asteroid populations provide a tracer for the dynamical evolution of the Solar System. The mission combines a long-range (point source) telescopic survey of over 10,000 objects, targeted close encounters with 10 – 20 asteroids and serendipitous searches to constrain the distribution of smaller (e.g. 10 m) size objects into a single concept. With a carefully targeted trajectory that loops through the asteroid belt, CASTAway would provide a comprehensive survey of the main belt at multiple scales. The scientific payload comprises a 50 cm diameter telescope that includes an integrated low-resolution (R = 30 – 100) spectrometer and visible context imager, a thermal (e.g. 6 – 16 μm) imager for use during the flybys, and modified star tracker cameras to detect small (~10 m) asteroids. The CASTAway spacecraft and payload have high levels of technology readiness and are designed to fit within the programmatic and cost caps for a European Space Agency medium class mission, whilst delivering a significant increase in knowledge of our Solar System.
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Can the European ELT detect super-Earths? Measuring the contrast limit of an image slicer spectrograph in a laboratory experiment

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9908 (2016) 99089r-99089r-8

Authors:

Robert M Barnsley, Matthias Tecza, Niranjan A Thatte
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Preliminary design study of the integral field unit for the E-ELT Harmoni instrument

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9908 (2016) 99089t-99089t-11

Authors:

J Kosmalski, M Tecza, I Bryson, F Clarke, D Freeman, M Loupias, JE Migniau, A Remillieux, NA Thatte
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Simulated observations of high-redshift galaxies with the HARMONI spectrograph for the European Extremely Large Telescope

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9908 (2016) 99089y-99089y-9

Authors:

Sarah Kendrew, Simon Zieleniewski, Ryan CW Houghton, Niranjan Thatte, Julien Devriendt, Matthias Tecza, Fraser Clarke, Kieran O'Brien, Boris Häußler
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