Utilizing the null stream of the Einstein Telescope
Evaluating data analysis challenges in the 3G detector era and discussing the solutions
Astrophysics, Data Analysis
My most recent work at the Gran Sasso Science Institute (GSSI) in Italy is focused on the development of new data analysis methods for the Einstein Telescope, a next-generation gravitational wave observatory planned for the 2030s. I defended my Ph.D. thesis at Monash University in Melbourne, Australia, and I worked for a short time at Swinburne University. Both institutes are a part of the OzGrav: the Centre of Excellence for Gravitational Wave Discovery. My Ph.D. thesis is titled "Neutron stars as gravitational wave emitters and detectors". The thesis is related to gravitational-wave searches with ground-based interferometers (LIGO) and pulsar timing arrays (PPTA). In 2015 I graduated with a joint B.Sc-M.Sc. degree from the Faculty of Physics of Lomonosov Moscow State University, where my work was on the gamma-ray burst instrumentation.
Recent Work
Utilizing the null stream of the Einstein Telescope
Common red process and gravitational waves
A precursor to the detection of nanohertz gravitational waves or unmodeled pulsar noise?
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