Public Release of the QuickCW Code

QuickCW v1.0.1

QuickCW is an analysis software dedicated to search for and characterize gravitational waves from individual supermassive black hole binaries (or continuous waves, CWs) in pulsar timing array data. It utilizes techniques from arXiv:2204.07160 and numba just-in-time compilation to make the code fast.

Read the documentation at: https://quickcw.readthedocs.io/en/latest/

Journal Citation

@ARTICLE{2022arXiv220407160B,
       author = {{B{\'e}csy}, Bence and {Cornish}, Neil J. and {Digman}, Matthew C.},
        title = "{Fast Bayesian analysis of individual binaries in pulsar timing array data}",
      journal = {arXiv e-prints},
     keywords = {General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2022,
        month = apr,
          eid = {arXiv:2204.07160},
        pages = {arXiv:2204.07160},
archivePrefix = {arXiv},
       eprint = {2204.07160},
 primaryClass = {gr-qc},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220407160B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}