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
Axelsson M
(2013)
Fast variability as a probe of the smallest regions around accreting black holes
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
Nebot Gómez-Morán A
(2013)
The XMM-Newton SSC survey of the Galactic plane
in Astronomy & Astrophysics
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
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
Sutton A
(2014)
Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources
in Monthly Notices of the Royal Astronomical Society
Basden A
(2014)
Faulty actuator tolerance in deformable mirrors for Extremely Large Telescope multi-object adaptive optics
in Monthly Notices of the Royal Astronomical Society
Basden A
(2014)
Wide-field adaptive optics performance in cosmological deep fields for multi-object spectroscopy with the European Extremely Large Telescope
in Monthly Notices of the Royal Astronomical Society
Basden A
(2014)
Real-time correlation reference update for astronomical adaptive optics
in Monthly Notices of the Royal Astronomical Society
Alston W
(2014)
X-ray time delays in the narrow line Seyfert 1 galaxy PG 1244+026
in Monthly Notices of the Royal Astronomical Society
{Abramowski}, A. And {Acero}, F. And {Aharonian}, F. And {Akhperjanian}, A.~G. And {Anton}, G. And {Balzer}, A. And {Barnacka}, A. And {Barres De Almeida}, U. And {Becherini}, Y. And {Becker}, J. And {Behera}, B. And {Bernl{\"o}hr}, K. And {Birsin}, E. And {Biteau}, J. And {Bochow}, A. And {Boisson}, C. And {Bolmont}, J. And {Bordas}, P. And {Brucker}, J. And {Brun}, F. And {Brun}, P. And {Bulik}, T. And {B{\"u}sching}, I. And {Carrigan}, S. And {Casanova}, S. And {Cerruti}, M. And {Chadwick},
(2014)
Erratum: ''Search for Dark Matter Annihilation Signals from the Fornax Galaxy Cluster with H.E.S.S.''
(2012, ApJ, 750, 123)
in \apj
Heida M
(2014)
Near-infrared counterparts of ultraluminous X-ray sources
in Monthly Notices of the Royal Astronomical Society
Hahn J
(2014)
Impact of aerosols and adverse atmospheric conditions on the data quality for spectral analysis of the H.E.S.S. telescopes
in Astroparticle Physics
Gardner E
(2014)
What powers the most relativistic jets? - I. BL Lacs
in Monthly Notices of the Royal Astronomical Society
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
Shepherd H
(2014)
Stereo-SCIDAR: optical turbulence profiling with high sensitivity using a modified SCIDAR instrument
in Monthly Notices of the Royal Astronomical Society
{H.~E.~S.~S.~Collaboration} And {Abramowski}, A. And {Aharonian}, F. And {Ait Benkhali}, F. And {Akhperjanian}, A.~G. And {Ang{\"u}ner}, E. And {Anton}, G. And {Backes}, M. And {Balenderan}, S. And {Balzer}, A. And Et Al.
(2014)
Search for extended {$\gamma$}-ray emission around AGN with H.E.S.S. and Fermi-LAT
in \aap
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
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
Basden A
(2014)
A real-time simulation facility for astronomical adaptive optics
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
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
Luangtip W
(2014)
A deficit of ultraluminous X-ray sources in luminous infrared galaxies
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 |