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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.

Christopher Williams

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  • 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.
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SETIBURST: A robotic, commensal, realtime multi-science backend for the Arecibo Telescope

Astrophysical Journal Supplement Series Institute of Physics 228:2 (2017) 21-21

Authors:

J Chennamangalam, D MacMahon, J Cobb, Aris Karastergiou, APV Siemion, K Rajwade, Wesley Armour, V Gajjar, MA McLaughlin, D Werthimer, Christopher Williams

Abstract:

Radio astronomy has traditionally depended on observatories allocating time to observers for exclusive use of their telescopes. The disadvantage of this scheme is that the data thus collected is rarely used for other astronomy applications, and in many cases, is unsuitable. For example, properly calibrated pulsar search data can, with some reduction, be used for spectral line surveys. A backend that supports plugging in multiple applications to a telescope to perform commensal data analysis will vastly increase the science throughput of the facility. In this paper, we present "SETIBURST," a robotic, commensal, realtime multi-science backend for the 305 m Arecibo Telescope. The system uses the 1.4 GHz, seven-beam Arecibo L-band Feed Array (ALFA) receiver whenever it is operated. SETIBURST currently supports two applications: SERENDIP VI, a SETI spectrometer that is conducting a search for signs of technological life, and ALFABURST, a fast transient search system that is conducting a survey of fast radio bursts (FRBs). Based on the FRB event rate and the expected usage of ALFA, we expect 0-5 FRB detections over the coming year. SETIBURST also provides the option of plugging in more applications. We outline the motivation for our instrumentation scheme and the scientific motivation of the two surveys, along with their descriptions and related discussions.
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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
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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
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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.
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