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.
Organisations
Publications
Jia P
(2015)
Simulation of atmospheric turbulence phase screen for large telescope and optical interferometer
in Monthly Notices of the Royal Astronomical Society
Collinson J
(2015)
Reaching the peak of the quasar spectral energy distribution - I. Observations and models
in Monthly Notices of the Royal Astronomical Society
Sutton A
(2015)
The hyperluminous X-ray source candidate in IC 4320: another HLX bites the dust
in Monthly Notices of the Royal Astronomical Society
Basden A
(2015)
Monte Carlo modelling of multiconjugate adaptive optics performance on the European Extremely Large Telescope
in Monthly Notices of the Royal Astronomical Society
Axelsson M
(2014)
An imperfect double: probing the physical origin of the low-frequency quasi-periodic oscillation and its harmonic in black hole binaries
in Monthly Notices of the Royal Astronomical Society
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
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
Jin C
(2013)
A long XMM-Newton observation of an extreme narrow-line Seyfert 1: PG 1244+026
in Monthly Notices of the Royal Astronomical Society
Gardner E
(2014)
What powers the most relativistic jets? - I. BL Lacs
in Monthly Notices of the Royal Astronomical Society
Soria R
(2019)
The discovery of weak coherent pulsations in the ultraluminous X-ray source NGC 1313 X-2
in Monthly Notices of the Royal Astronomical Society: Letters
Middleton M
(2013)
Broad absorption features in wind-dominated ultraluminous X-ray sources?
in Monthly Notices of the Royal Astronomical Society: Letters
Algorri JF
(2013)
Modal liquid crystal array of optical elements.
in Optics express
MacLachlan DG
(2016)
Development of integrated mode reformatting components for diffraction-limited spectroscopy.
in Optics letters
Abramowski A
(2013)
Constraints on axionlike particles with H.E.S.S. from the irregularity of the PKS 2155 - 304 energy spectrum
in Physical Review D
Yamada S
(2013)
Evidence for a Cool Disk and Inhomogeneous Coronae from Wide-Band Temporal Spectroscopy of Cygnus X-1 with Suzaku
in Publications of the Astronomical Society of Japan
Tomsick J
(2015)
THE ACCRETING BLACK HOLE SWIFT J1753.5-0127 FROM RADIO TO HARD X-RAY
in The Astrophysical Journal
D'Abrusco R
(2014)
THE TWO-DIMENSIONAL SPATIAL DISTRIBUTIONS OF THE GLOBULAR CLUSTERS AND LOW-MASS X-RAY BINARIES OF NGC 4649
in The Astrophysical Journal
Gandhi P
(2013)
REFLECTION-DOMINATED NUCLEAR X-RAY EMISSION IN THE EARLY-TYPE GALAXY ESO 565-G019
in The Astrophysical Journal
Prestwich A
(2013)
ULTRA-LUMINOUS X-RAY SOURCES IN THE MOST METAL POOR GALAXIES
in The Astrophysical Journal
Yamada S
(2013)
HIGHLY IONIZED Fe-K ABSORPTION LINE FROM CYGNUS X-1 IN THE HIGH/SOFT STATE OBSERVED WITH SUZAKU
in The Astrophysical Journal
Sutton A
(2015)
X-RAY SPECTRAL RESIDUALS IN NGC 5408 X-1: DIFFUSE EMISSION FROM STAR FORMATION, OR THE SIGNATURE OF A SUPER-EDDINGTON WIND?
in The Astrophysical Journal
Earnshaw H
(2020)
The (Re)appearance of NGC 925 ULX-3, a New Transient ULX
in The Astrophysical Journal
Aliu E
(2013)
LONG-TERM TeV AND X-RAY OBSERVATIONS OF THE GAMMA-RAY BINARY HESS J0632+057
in The Astrophysical Journal
Shidatsu M
(2013)
THE ACCRETION DISK AND IONIZED ABSORBER OF THE 9.7 hr DIPPING BLACK HOLE BINARY MAXI J1305-704
in The Astrophysical Journal
Walton D
(2013)
X-RAY OUTFLOWS AND SUPER-EDDINGTON ACCRETION IN THE ULTRALUMINOUS X-RAY SOURCE HOLMBERG IX X-1
in The Astrophysical Journal
Hori T
(2014)
ERRATUM: " SUZAKU OBSERVATION OF THE BLACK HOLE BINARY 4U 1630-47 IN THE VERY HIGH STATE" (2014, ApJ, 790, 20)
in The Astrophysical Journal
Gladstone J
(2013)
OPTICAL COUNTERPARTS OF THE NEAREST ULTRALUMINOUS X-RAY SOURCES
in The Astrophysical Journal Supplement Series
Heida M
(2014)
Near-infrared counterparts of ultraluminous X-ray sources
Luangtip W
(2014)
A deficit of ultraluminous X-ray sources in luminous infrared galaxies
Middleton M
(2013)
Broad absorption features in wind-dominated ULXs?
Sathyaprakash R
(2019)
Observational limits on the X-ray emission from the bubble nebula surrounding Ho IX X-1
Earnshaw H
(2020)
The (re)appearance of NGC 925 ULX-3, a new transient ULX
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 |