51猎奇入口

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • 51猎奇入口
    • Undergraduates
    • Postgraduates
  • Engage
    • For young people
    • For teachers
    • For the public
    • For alumni
    • For business
  • Support
Menu
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.

Christopher Williams

Visitor

Sub department

  • Astrophysics
Christopher.Williams@physics.ox.ac.uk
  • About
  • Publications

ALFABURST: A realtime fast radio burst monitor for the Arecibo telescope

The Fourteenth Marcel Grossmann Meeting World Scientific Publishing Co (2017) 2872-2876

Authors:

Jayanth Chennamangalam, Aris Karastergiou, David MacMahon, Wesley G Armour, Jeff Cobb, Duncan Lorimer, Kaustubh Rajwade, Andrew Siemion, Dan Werthimer, Christopher Williams

Abstract:

Fast radio bursts (FRBs) constitute an emerging class of fast radio transient whose origin continues to be a mystery. Realizing the importance of increasing coverage of the search parameter space, we have designed, built, and deployed a realtime monitor for FRBs at the 305-m Arecibo radio telescope. Named `ALFABURST', it is a commensal instrument that is triggered whenever the 1.4 GHz seven-beam Arecibo L-Band Feed Array (ALFA) receiver commences operation. The ongoing commensal survey we are conducting using ALFABURST has an instantaneous field of view of 0.02 sq. deg. within the FWHM of the beams, with the realtime software configurable to use up to 300 MHz of bandwidth. We search for FRBs with dispersion measure up to 2560 cm^-3 pc and pulse widthsranging from 0.128 ms to 16.384 ms. Commissioning observations performed over the past few months have demonstrated the capability of the instrument in detecting single pulses from known pulsars. In this paper, I describe the instrument and the associated survey.

SETIBURST: A Robotic, Commensal, Realtime Multi-science Backend for the Arecibo Telescope

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 228:2 (2017) ARTN 21

Authors:

J Chennamangalam, D MacMahon, J Cobb, A Karastergiou, APV Siemion, K Rajwade, W Armour, V Gajjar, DR Lorimer, MA McLaughlin, D Werthimer, C Williams

ARTEMIS: A real-time data processing pipeline for the detection of fast transients

Institute of Electrical and Electronics Engineers (IEEE) (2015) 1-1

Authors:

Jayanth Chennamangalam, Aris Karastergiou, Wes Armour, Christopher Williams, Mike Giles

Limits on fast radio bursts at 145 MHz with ARTEMIS, a real-time software backend

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 452:2 (2015) 1254-1262

Authors:

A Karastergiou, J Chennamangalam, W Armour, C Williams, B Mort, F Dulwich, S Salvini, A Magro, S Roberts, M Serylak, A Doo, AV Bilous, RP Breton, H Falcke, J-M Griessmeier, JWT Hessels, EF Keane, VI Kondratiev, M Kramer, J van Leeuwen, A Noutsos, S Oslowski, C Sobey, BW Stappers, P Weltevrede

Flexible services for the support of research.

Philos Trans A Math Phys Eng Sci 371:1983 (2013) 20120067

Authors:

Matteo Turilli, David Wallom, Chris Williams, Steve Gough, Neal Curran, Richard Tarrant, Dan Bretherton, Andy Powell, Matt Johnson, Terry Harmer, Peter Wright, John Gordon

Abstract:

Cloud computing has been increasingly adopted by users and providers to promote a flexible, scalable and tailored access to computing resources. Nonetheless, the consolidation of this paradigm has uncovered some of its limitations. Initially devised by corporations with direct control over large amounts of computational resources, cloud computing is now being endorsed by organizations with limited resources or with a more articulated, less direct control over these resources. The challenge for these organizations is to leverage the benefits of cloud computing while dealing with limited and often widely distributed computing resources. This study focuses on the adoption of cloud computing by higher education institutions and addresses two main issues: flexible and on-demand access to a large amount of storage resources, and scalability across a heterogeneous set of cloud infrastructures. The proposed solutions leverage a federated approach to cloud resources in which users access multiple and largely independent cloud infrastructures through a highly customizable broker layer. This approach allows for a uniform authentication and authorization infrastructure, a fine-grained policy specification and the aggregation of accounting and monitoring. Within a loosely coupled federation of cloud infrastructures, users can access vast amount of data without copying them across cloud infrastructures and can scale their resource provisions when the local cloud resources become insufficient.

Pagination

  • First page First
  • Previous page Prev
  • Page 1
  • Page 2
  • Page 3
  • Current page 4
  • Page 5
  • Page 6
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • 51猎奇入口
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • 51猎奇入口
  • Giving to Physics