PESSTO: survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects⋆⋆⋆
Astronomy & Astrophysics EDP Sciences 579 (2015) a40
The peculiar radio galaxy 4C 35.06: a case for recurrent AGN activity?
Astronomy & Astrophysics EDP Sciences 579 (2015) a27
Particle acceleration and magnetic field amplification in the jets of 4C74.26
Astrophysical Journal American Astronomical Society 806:2 (2015) ARTN 243
Abstract:
We model the multi-wavelength emission in the southern hotspot of the radio quasar 4C74.26. The synchrotron radio emission is resolved near the shock with the MERLIN radio-interferometer, and the rapid decay of this emission behind the shock is interpreted as the decay of the amplified downstream magnetic field as expected for small scale turbulence. Electrons are accelerated to only 0.3 TeV, consistent with a diffusion coefficient many orders of magnitude greater than in the Bohm regime. If the same diffusion coefficient applies to the protons, their maximum energy is only ~100 TeV.Radio monitoring of the hard state jets in the 2011 outburst of MAXI J1836−194
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 450:2 (2015) 1745-1759
LORD OF THE RINGS: A KINEMATIC DISTANCE TO CIRCINUS X-1 FROM A GIANT X-RAY LIGHT ECHO
The Astrophysical Journal American Astronomical Society 806:2 (2015) 265