A possible precursor for the detection of nanohertz gravitational waves or unmodeled pulsar noise?
My most recent work is focused on the development of new data analysis methods for the Einstein Telescope. Prior to starting my position at the GSSI, I worked at Swinburne University with Prof. Ryan Shannon on the search for the nanohertz-frequency gravitational-wave background with pulsar timing arrays. In 2020 I have been awarded a Ph.D. degree at Monash University, where I worked withand . My thesis is titled " ". The thesis is related to gravitational-wave searches with ground-based interferometers ( ) and pulsar timing arrays ( ). In 2015 I graduated with a Specialist Degree from the Faculty of Physics of Lomonosov Moscow State University, where I worked on calibration of space-based gamma-ray burst detectors for the .
We model red noise and link exponential dips in residuals with pulse shape changes