Harvard Prize Postdoctoral Fellow | Caltech Astrophysics PhD
My work primarily relies on a multiwavelength crossmatch between X-rays from the SRG/eROSITA mission and optical data from the Zwicky Transient Facility and Gaia, though I also use data from other X-ray, optical, and radio telescopes. I am broadly interested in applying statistical techniques to extract scientific results out of large astronomical datasets, and have shown that a simple tool, the “X-ray Main Sequence”, can efficiently reveal the true demographics of accreting white dwarfs in the solar neighborhood.
Long period radio transients (LPTs) have been the first new class of radio pulsators in decades. Until now, pulsars and millisecond pulsars have occupied the sub-period regime, while LPTs exhibit radio pulse periods on the order of minutes to hours.
