My research field is focussed on timing- and imaging aspects
of X-ray/gamma-ray pulsars and high-energy transients.
In particular, I use data from a wide variety of high-energy
instruments aboard space-borne satellites like NICER, NuSTAR,
XMM-Newton, Chandra, Swift-XRT, INTEGRAL, Fermi-GBM/LAT,
Insight-HXMT and IXPE to do this research.
Coded mask maximum likelihood imaging studies are performed
for the WFM (2-50 keV) configuration aboard eXTP and Strobe-X.
