Posted in astro-ph.HE · 2026-08-18 · Andrew R. Kaiser, Jeffrey S. Hazboun, Maura A. McLaughlin, H. Thankful Cromartie, Emmanuel Fonseca, Joseph Simon, Stephen R. Taylor, Michele Vallisneri, Sarah J. Vigeland, Zaven Arzoumanian, Paul T. Baker, Harsha Blumer, Paul R. Brook, Ismael Cognard, Megan E. DeCesar, Paul B. Demorest, Timothy Dolch, F. Adam Dong, Justin A. Ellis, Robert D. Ferdman, Elizabeth C. Ferrara, William Fiore, Nate Garver-Daniels, Peter A. Gentile, Deborah C. Good, Lucas Guillemot, Ross J. Jennings, Megan L. Jones, David L. Kaplan, Victoria M. Kaspi, Matthew Kerr, Aida Yu. Kirichenko, Michael T. Lam, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Alexander McEwen, James W. McKee, Natasha McMann, Bradley W. Meyers, Arun Naidu, Cherry Ng, David J. Nice, Aditya Parthasarathy, Timothy T. Pennucci, Benetge B. P. Perera, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Brent J. Shapiro-Albert, Renée Spiewak, Ingrid H. Stairs, Kevin Stovall, Joseph K. Swiggum, Chia Min Tan, Shriharsh P. Tendulkar, Haley M. Wahl, WeiWei Zhu
In this study, we use the Bayesian methods in the Enterprise package to examine the fully general parameterization of pulsar timing models in tandem with noise. We investigate four pulsars, PSR J1600$-$3053, PSR J2043+1711, PSR J0740+6620, and PSR J1640+2224, through the lens of Bayesian timing. These four are selected as they are...