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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 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.

Prof Michael Jones

Professor of Experimental Cosmology

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Cosmology
  • Experimental radio cosmology
  • C-BASS
  • The Square Kilometre Array (SKA)
Mike.Jones@physics.ox.ac.uk
Telephone: 01865 (2)73441
Denys Wilkinson Building, room 758
  • About
  • Publications

The STRIP instrument of the Large Scale Polarization Explorer: microwave eyes to map the Galactic polarized foregrounds

SPIE, the international society for optics and photonics 10708 (2018) 107081g

Authors:

Cristian Franceschet, Sabrina Realini, Aniello Mennella, Giuseppe Addamo, Alessandro Ba霉, Paola M Battaglia, Marco Bersanelli, Barbara Caccianiga, Silvia Caprioli, Francesco Cavaliere, Kieran A Cleary, Francesco Cuttaia, Francesco Del Torto, Viviana Fafone, Zunnoorain Farooqui, Ricardo T G茅nova Santos, Todd C Gaier, Massimo Gervasi, Tommaso Ghigna, Federico Incardona, Simone Iovenitti, Mike Jones, Pekka Kangaslahti, Roberto Mainini, Davide Maino, Michele Maris, Patricio Mena, Roc铆o Molina, Gianluca Morgante, Andrea Passerini, Maria del Rosario Perez-de-Taoro, Oscar A Peverini, Federico Pezzotta, Claudio Pincella, Nicol谩s Reyes, Alessio Rocchi, Jos茅 A Rubi帽o-Mart铆n, Maura Sandri, Stefano Sartor, Mary Soria, Valeria Tapia, Luca Terenzi, Maurizio Tomasi, Elisabetta Tommasi, Daniele M Vigan贸, Fabrizio Villa, Giuseppe Virone, Angela Volpe, Bob Watkins, Andrea Zacchei, Mario Zannoni

A compact quad-ridge orthogonal mode transducer with wide operational bandwidth

IEEE Antennas and Wireless Propagation Letters Institute of Electrical and Electronics Engineers 17:3 (2018) 422-425

Authors:

Alexander Pollak, Michael E Jones

Abstract:

We present the design and the measured performance of a compact quad-ridge orthomode transducer (OMT) operating in C-band with more than 100% fractional bandwidth. The OMT comprises two sets of identical orthogonal ridges mounted in a circular waveguide. The profile of these ridges was optimised to reduce significantly the transition length, while retaining the wide operational bandwidth of the quad-ridge OMT. In this letter, we show that the optimised compact OMT has better than -15dB return loss with the cross-polarisation well below -40dB in the designated 4.0-8.5GHz band.

The Low Frequency Receivers for SKA1-Low: Design and Verification

Institute of Electrical and Electronics Engineers (IEEE) (2017) 1-4

Authors:

Pieter Benthem, Marchel Gerbers, Jan Geralt Bij de Vaate, Stefan Wijnholds, Jeanette Bast, Tom Booler, Tim Colgate, Brian Crosse, David Emrich, Peter Hall, Budi Juswardy, David Kenney, Franz Schlazenhaufer, Marcin Sokolowski, Adrian Sutinjo, Daniel Ung, Randall Wayth, Andrew Williams, Monica Alderighi, Pietro Bolli, Gianni Comoretto, Andrea Mattana, Jader Monari, Giovanni Naldi, Frederico Perini, Giuseppe Pupillo, Simone Rusticelli, Marco Schiaffino, Francesco Schilliro, Amin Aminei, Riccardo Chiello, Mike Jones, Jeremy Baker, Richard Bennett, Rob Halsall, Georgina Kaligeridou, Matthew Roberts, Hermine Schnetler, Jens Abraham, Eloy De Lera Accdo, Andrew Faulkner, Nima Razavi Ghods, Denis Cutajar, Andrea DeMarco, Alessio Magro, Kristian Zarb Adami

HIPSR: A digital signal processor for the Parkes 21-cm multibeam receiver

Journal of Astronomical Instrumentation World Scientific Publishing 5:4 (2016)

Authors:

DC Price, L Staveley-Smith, M Bailes, E Carretti, A Jameson, Michael Jones, W van Straten, SW Schediwy

Abstract:

HIPSR (HI-Pulsar) is a digital signal processing system for the Parkes 21-cm Multibeam Receiver that provides larger instantaneous bandwidth, increased dynamic range, and more signal processing power than the previous systems in use at Parkes. The additional computational capacity enables finer spectral resolution in wideband HI observations and real-time detection of Fast Radio Bursts during pulsar surveys. HIPSR uses a heterogeneous architecture, consisting of FPGA-based signal processing boards connected via high-speed Ethernet to high performance compute nodes. Low-level signal processing is conducted on the FPGA-based boards, and more complex signal processing routines are conducted on the GPU-based compute nodes. The development of HIPSR was driven by two main science goals: to provide large bandwidth, high-resolution spectra suitable for 21-cm stacking and intensity mapping experiments; and to upgrade the Berkeley鈥揚arkes鈥揝winburne Recorder (BPSR), the signal processing system used for the High Time Resolution Universe (HTRU) Survey and the Survey for Pulsars and Extragalactic Radio Bursts (SUPERB).

Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz

Monthly Notices of the Royal Astronomical Society 91探花 University Press (OUP) 453:2 (2015) 2082-2093

Authors:

C Demetroullas, C Dickinson, D Stamadianos, SE Harper, K Cleary, Michael E Jones, TJ Pearson, ACS Readhead, Angela C Taylor

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