Jeffrey S. Hazboun, Joseph Simon, jeremy baier, Bjorn Larsen, Daniel J Oliver, Paul T. Baker, Bence Bécsy, Siyuan Chen, Alberto Diaz Hernandez, Justin A. Ellis, A. M. Holgado, Kristina Islo, Aaron Johnson, Andrew R. Kaiser, Nima Laal, Alexander McEwen, Nihan S. Pol, Joey Shapiro Key, Min Young Kim, Matthew Samson, Brent J. Shapiro-Albert, Jerry P. Sun, Stephen R. Taylor, Caitlin A. Witt, Jeremy Volpe, Christine Ye, Harsha Blumer, Paul R. Brook, Shami Chatterjee, James M. Cordes, Fronefield Crawford, H. Thankful Cromartie, Megan E. DeCesar, Paul B. Demorest, Timothy Dolch, Robert D. Ferdman, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, N. Garver-Daniels, Peter A. Gentile, Deborah C. Good, Ross J. Jennings, Megan L. Jones, David L. Kaplan, Michael T. Lam, T. Joseph W. Lazio, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Dustin R. Madison, Maura A. McLaughlin, Chiara M. F. Mingarelli, Cherry Ng, David J. Nice, Timothy T. Pennucci, Scott M. Ransom, Paul S. Ray, Xavier Siemens, Renée Spiewak, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Joseph K. Swiggum, Jacob E. Turner, Michele Vallisneri, Sarah J. Vigeland
Abstract Pulsar timing arrays (PTAs) have recently entered the detection era, quickly moving beyond the goal of simply improving sensitivity at the lowest frequencies for the sake of observing the stochastic gravitational wave background (GWB), and focusing on its accurate spectral characterization. While all PTA collaborations around the world use Fourier-domain Gaussian processes to model the GWB and intrinsic long time-correlated (red) noise, techniques to model the time-correlated radio-frequency-dependent (chromatic) processes have varied from collaboration to collaboration. Here we test a new class of models for PTA data, Gaussian processes based on time-domain kernels that model the statistics of the chromatic processes starting from the covariance matrix. As we will show, these models can be effectively equivalent to Fourier-domain models in mitigating chromatic noise. This work presents a method for Bayesian model selection across the various choices of kernel as well as deterministic chromatic models for nonstationary chromatic events and the solar wind. As PTAs turn toward high frequency (>1 yr −1 ) sensitivity, the size of the basis used to model these processes will need to increase, and these time-domain models present some computational efficiencies compared to Fourier-domain models.