Antonio (Tony) C. Rodriguez

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Harvard Prize Postdoctoral Fellow | Caltech Astrophysics PhD

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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

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.

GLEAM-X J0704-37

Accreting White Dwarfs (Cataclysmic Variables)

Ultracompact White Dwarfs and Gravitational Waves (AM CVn Binaries)

Stellar-Mass Black Holes

Gravitational Microlensing