The Arcminute Microkelvin Imager Catalogue of Gamma-ray Burst afterglows at 15.7 GHz

(2017)

Authors:

GE Anderson, TD Staley, AJ van der Horst, RP Fender, A Rowlinson, KP Mooley, JW Broderick, RAMJ Wijers, C Rumsey, DJ Titterington

Up and Down the Black Hole Radio/X-ray Correlation: the 2017 mini-outbursts from Swift J1753.5-0127

(2017)

Authors:

RM Plotkin, J Bright, JCA Miller-Jones, AW Shaw, JA Tomsick, TD Russell, G-B Zhang, DM Russell, RP Fender, J Homan, P Atri, F Bernardini, JD Gelfand, F Lewis, TM Cantwell, SH Carey, KJB Grainge, J Hickish, YC Perrott, N Razavi-Ghods, AMM Scaife, PF Scott, DJ Titterington

Paving the way to simultaneous multi-wavelength astronomy

(2017)

Authors:

MJ Middleton, P Casella, P Gandhi, E Bozzo, G Anderson, N Degenaar, I Donnarumma, G Israel, C Knigge, A Lohfink, S Markoff, T Marsh, N Rea, S Tingay, K Wiersema, D Altamirano, D Bhattacharya, WN Brandt, S Carey, P Charles, M Diaz Trigo, C Done, M Kotze, S Eikenberry, R Fender, P Ferruit, F Fuerst, J Greiner, A Ingram, L Heil, P Jonker, S Komossa, B Leibundgut, T Maccarone, J Malzac, V McBride, J Miller-Jones, M Page, EM Rossi, DM Russell, T Shahbaz, GR Sivakoff, M Tanaka, DJ Thompson, M Uemura, P Uttley, G van Moorsel, M Van Doesburgh, B Warner, B Wilkes, J Wilms, P Woudt

Gamma-ray and X-ray emission from the Galactic Centre: hints on the nuclear star cluster formation history

(2017)

Authors:

Manuel Arca-Sedda, Bence Kocsis, Timothy Brandt

Cosmic ray acceleration by relativistic shocks: Limits and estimates

Monthly Notices of the Royal Astronomical Society Oxford University Press (2017)

Authors:

AR Bell, AT Araudo, James H Matthews, Katherine M Blundell

Abstract:

We examine limits to the energy to which cosmic rays can be accelerated by relativistic shocks, showing that acceleration of light ions as high as 100 EeV is unlikely. The implication of our estimates is that if ultra-high energy cosmic rays are accelerated by shocks, then those shocks are probably not relativistic.