About Me

My Research

Recorded Talks and Press

Overview

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.

A New Class of Radio-pulsing Sources: Long Period Radio Transients

Accreting White Dwarfs (Cataclysmic Variables)

Ultracompact White Dwarfs and Gravitational Waves (AM CVn Binaries)

Stellar-Mass Black Holes

Gravitational Microlensing