This code lays the foundations for constructing synthetic time-frequency data from a millisecond pulsar orbiting a massive black hole (e.g. Galactic centre). See also Pulsar timing in extreme mass ratio binaries: a general relativistic approach

Tom Kimpson
Tom Kimpson
Ph.D. Candidate, Theoretical Astrophysics

My research interests include high energy astrophysics and gravitational wave astronomy.