Parameters of gravitational waveforms for compact binary coalescences: masses, spins, etc.
A possible precursor for the detection of nanohertz gravitational waves or unmodeled pulsar noise?
We model red noise and link exponential dips in residuals with pulse shape changes
Understanding millisecond pulsar spin noise and neutron star physics
Some useful tips for writing papers with LaTeX markup language and Overleaf
Installation of Tempo2, Libstempo, Enterprise. Timing residuals PSD and Lomb-Scargle method.
Formulae for binary evolution, etc. The list will get replenished with time.
Basic commands and tips: how to use terminal on Mac, to run a program in terminal, what is bash, etc.
Here I collect some useful python commands for code development
A description of known sources of signals and noise in Pulsar Timing Array experiments
Installing programs and packages, running Jupyter notebook, parallel computing with Slurm
Artist's sketch of accreting neutron star, a possible source of gravitational waves. Image: NASA.
This page explains how to work with MATLAB R2015a (220.127.116.11613) 64-bit (glnxa64).
Visual representation of two merging neutron stars. Image: NASA.
LIGO data structure: job files, frames, calibrations, for preproc.m (STAMP) and stochastic.m.
Artist's representation of a GRB jets (NASA), and a 3D model of the Lomonosov satellite (MSU).