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The Sleeping Monster: NuSTAR observations of SGR 1806-20, 11 years after the Giant Flare
George Younes, Matthew G. Baring, Chryssa Kouveliotou +5
We report the analysis of 5 NuSTAR observations of SGR 1806-20 spread over a year from April 2015 to April 2016, more than 11 years following its Giant Flare (GF) of 2004. The sour…
X-ray Synchrotron Polarization from Turbulent Plasmas in Supernova Remnants
Matthew G. Baring
As supernova remnants (SNRs) age, they become efficient cosmic ray accelerators at their outer shell shocks. The current paradigm for shock acceleration theory favors turbulent fie…
Magnetar Hard Spectral Tails
Zorawar Wadiasingh, Matthew G. Baring, Peter L. Gonthier +1
Pulsed non-thermal quiescent emission between 10 keV and around 150 keV has been observed in magnetars. For inner magnetospheric models of such hard X-ray signals, resonan…
Hard X-ray Quiescent Emission in Magnetars via Resonant Compton Upscattering
M. G. Baring, Z. Wadiasingh, P. L. Gonthier +1
Non-thermal quiescent X-ray emission extending between 10 keV and around 150 keV has been seen in about 10 magnetars by RXTE, INTEGRAL, Suzaku, NuSTAR and Fermi-GBM. For inner magn…