@article{2a18abb25acc4dcd8aeebf1bb615bba8,
title = "On the free precession candidate PSR B1828−11: Evidence for increasing deformation",
keywords = "Methods: data analysis, Pulsars: individual: PSR B1828−11, Stars: neutron",
author = "G. Ashton and Jones, {D. I.} and R. Prix",
note = "Funding Information: GA acknowledges financial support from the University of Southampton and the Albert Einstein Institute (Hannover). DIJ acknowledges support from STFC via grant number ST/H002359/1, and also travel support from NewCompStar (a COST-funded Research Networking Programme). We thank Nils Andersson for comments on this manuscript, Betina Posselt for advice on setting limits on X-ray flux, Foreman-Mackey et al. (2014) for the software used in generating posterior probability distributions and Lyne et al. (2010) for generously sharing the data for PSR B1828−11. Publisher Copyright: {\textcopyright} 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society",
year = "2017",
month = may,
doi = "10.1093/mnras/stx060",
language = "English",
volume = "467",
pages = "164--178",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "1",
}