Publications

The UTMOST: A hybrid digital signal processor transforms the MOST 

M. Bailes, A. Jameson, C. Flynn, T. Bateman, E. D. Barr, S. Bhandari, J. D. Bunton, M. Caleb, D. Campbell-Wilson, W. Farah, B. Gaensler, A. J. Green, R. W. Hunstead, F. Jankowski, E. F. Keane, V. Venkatraman Krishnan, Tara Murphy, M. O’Neill, S. Oslowski, A. Parthasarathy, V. Ravi, P. Rosado, D. Temby https://arxiv.org/abs/1708.09619

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The first interferometric detections of Fast Radio Bursts

M. Caleb, C. Flynn, M. Bailes, E.D. Barr, T. Bateman, S. Bhandari, D. Campbell-Wilson, W. Farah, A.J. Green, R.W. Hunstead, A. Jameson, F. Jankowski, E.F. Keane, A. Parthasarathy, V. Ravi, P.A. Rosado, W. van Straten, V. Venkatraman Krishnan https://arxiv.org/abs/1703.10173

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Fast Radio Transient searches with UTMOST at 843 MHz

M. Caleb, C. Flynn, M. Bailes, E. D. Barr, T. Bateman, S. Bhandari, D. Campbell-Wilson, A. J. Green, R. W. Hunstead, A. Jameson, F. Jankowski, E. F. Keane, V. Ravi, W. van Straten, V. Venkataraman Krishnan https://arxiv.org/abs/1601.02444

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Just over 24 hours search data for FRBs at Molonglo. FRB candidates are shown as blue circles, and the bright pulsars Vela (magenta) and J1644-4559 (orange) are shown transiting the search region on the telescope meridian. Over 500 hours of search data have been used to set new upper limits on the FRB rate at 843 MHz.


 

Are the distributions of Fast Radio Burst properties consistent with a cosmological population? M.Caleb, C.Flynn, M.Bailes, E.D.Barr, R.W.Hunstead, E.F.Keane, V.Ravi, W. van Straten (2015). http://arxiv.org/abs/1512.02738

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Distributions in simulations of the slope of the logN-LogS relation for FRBs in two models of their comoving densities in LCDM cosmologies. The distributions are found to be consistent with observations of FRBs in the HILAT survey conducted at Parkes Radio Telescope, and thus consistent with them being of cosmological origin.

 

The NuSTAR view of the non-thermal emission from PSR J0437-4715. Guillot et al (2015). http://arxiv.org/abs/1512.03957

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Molonglo’s ephemeris for the bright Southern hemisphere millisecond pulsar was used to make a detection of the pulsed emission in X-rays with the NuSTAR satellite.

 

Glitch event observed in the Vela pulsar (PSR J0835-4510). Jankowski et alia 2015. Astronomer’s Telegram #6903. 

glitch1 (1)

Glitch event observed in the pulsar PSR J1740-3015. Jankowski et alia 2015. Astronomer’s Telegram #8298. 

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