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QuickCW

Fast continuous wave (CW) analysis for pulsar timing array data.

See arXiv:2204.07160 for details on the method, and the Quick-start Guide for details on how to run the code yourself!

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}
}

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Fast continuous wave (CW) analysis for PTA data

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