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A Programme of Astronomical Instrumentation and High-Energy Astrophysics at Durham 2013-2015

Lead Research Organisation: Durham University
Department Name: Physics

Abstract

We propose to consolidate our successful rolling programme of research and development in astronomical instrumentation for ground- and space-based telescopes with observational and theoretical work in high-energy astrophysics. Over the period 2013-2015 we will make high-fidelity laboratory experiments to assess the applicability of adaptive optics correction down to visible wavelengths, and exploit data from vertical turbulence profiling equipment to study the effects of low-altitude turbulence on telescope performance. We will also continue our joint programme with ESO to develop the next generation of real-time control systems for future adaptive optics systems, and undertake a development programme using our in-house manufacturing capability to deliver high-precision large-diameter diamond-machined optics for next-generation instruments. We will explore the application of photonics technologies to improving the versatility and efficiency of future astronomical spectrographs using fibre switches and image-stabilising optics. Our rolled up high energy astrophysics programme will use data from new hard X-ray satellites to study extreme accretion flows around compact objects, and will develop an outreach programme for the next-generation high energy gamma ray facility, the Cherenkov Telescope Array.

Planned Impact

The research will benefit UK astronomers by providing them with new technologies for implementing advanced modes of astronomical adaptive optics and improving the efficiency of optical/infrared spectroscopy. Astronomers worldwide will benefit from the synergy with technology developments at other observatories. Industry will benefit from cutting-edge developments of their systems (particularly real-time computing) and in supplying COTS items to the programme. The field of high-energy astrophysics will be moved forward by access to new data from hard X-ray telescopes, and by an effective outreach programme for CTA which helps secure future UK involvement.

Publications

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Jia P (2015) Simulation of atmospheric turbulence phase screen for large telescope and optical interferometer in Monthly Notices of the Royal Astronomical Society

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Basden A. G. (2017) On-sky demonstration of matched filters for wavefront measurements using ELT-scale elongated laser guide stars in Monthly Notices of the Royal Astronomical Society

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Sathyaprakash R (2022) A multi-wavelength view of distinct accretion regimes in the pulsating ultraluminous X-ray source NGC 1313 X-2 in Monthly Notices of the Royal Astronomical Society

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Jia P (2015) Real-time generation of atmospheric turbulence phase screen with non-uniform fast Fourier transform in Monthly Notices of the Royal Astronomical Society

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Heida M (2014) Near-infrared counterparts of ultraluminous X-ray sources in Monthly Notices of the Royal Astronomical Society

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Harris R (2015) Photonic spatial reformatting of stellar light for diffraction-limited spectroscopy in Monthly Notices of the Royal Astronomical Society

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MacLachlan D (2017) Efficient photonic reformatting of celestial light for diffraction-limited spectroscopy in Monthly Notices of the Royal Astronomical Society

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Gardner E (2013) Jets and the accretion flow in low-luminosity black holes in Monthly Notices of the Royal Astronomical Society

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Föhring D (2013) ULTRACAM z'-band detection of the secondary eclipse of WASP-12b in Monthly Notices of the Royal Astronomical Society

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Hagino K (2015) The origin of ultrafast outflows in AGN: Monte Carlo simulations of the wind in PDS 456 in Monthly Notices of the Royal Astronomical Society

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Kolehmainen M (2014) The soft component and the iron line as signatures of the disc inner radius in Galactic black hole binaries in Monthly Notices of the Royal Astronomical Society

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Bitenc U (2015) On-sky tests of the CuReD and HWR fast wavefront reconstruction algorithms with CANARY in Monthly Notices of the Royal Astronomical Society

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Sutton A (2014) Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources in Monthly Notices of the Royal Astronomical Society

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Barr D (2015) Reducing adaptive optics latency using Xeon Phi many-core processors in Monthly Notices of the Royal Astronomical Society

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Luangtip W (2015) A deficit of ultraluminous X-ray sources in luminous infrared galaxies in Monthly Notices of the Royal Astronomical Society

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Catala L (2013) Optical turbulence characterization at the SAAO Sutherland site in Monthly Notices of the Royal Astronomical Society

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Starling R (2014) The story of Seyfert galaxy RE J2248-511: from intriguingly ultrasoft to unremarkably average in Monthly Notices of the Royal Astronomical Society

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Sathyaprakash R (2019) Observational limits on the X-ray emission from the bubble nebula surrounding Ho IX X-1 in Monthly Notices of the Royal Astronomical Society

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Basden A (2014) A real-time simulation facility for astronomical adaptive optics in Monthly Notices of the Royal Astronomical Society

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Done C (2013) A new way to measure supermassive black hole spin in accretion disc-dominated active galaxies in Monthly Notices of the Royal Astronomical Society

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Osborn J (2015) Atmospheric scintillation in astronomical photometry in Monthly Notices of the Royal Astronomical Society

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Earnshaw H (2016) A variable ULX and possible IMBH candidate in M51a in Monthly Notices of the Royal Astronomical Society

 
Description This bridging award enabled a continued programme of underpinning research in 4 key areas of (i) adaptive optics, (ii) atmospheric characterisation, (iii) real-time control systems, (iv) 3D imaging and spectroscopy. One area research programme on freeform optics manufacture was not supported. Key findings are listed in the publications (especially SPIE) associated with this grant.
Exploitation Route The outcomes of this award fed directly into a continuing programme of technology development funded as part of our first Consolidated Grant.
Sectors Aerospace

Defence and Marine