Image Details

Choose export citation format:

RM-Tools: Software for Analyzing Polarized Radio Spectra

  • Authors: Cameron L. Van Eck, Cormac R. Purcell, Lerato Baidoo, Alec J. M. Thomson, Yik Ki Ma, Lindsey Oberhelman, Erik Osinga, Shannon Vanderwoude, Jennifer L. West, Shinsuke Ideguchi, Dylan M. Paré, Jane F. Kaczmarek, Tony Willis, Takuya Akahori, Craig S. Anderson, B. M. Gaensler, Shane O'Sullivan, Xiaohui Sun, Ariel D. Amaral, C. J. Riseley, Jeroen Stil, Xiang Zhang

Cameron L. Van Eck et al 2026 The Astrophysical Journal Supplement Series 283 .

  • Provider: AAS Journals

Caption: Figure 1.

Top-left panel: residual q/σq and u/σu spectra of a simple (blue) and complex (red) source after a Faraday thin model derived from RM-synthesis has been subtracted. Dashed lines show the ±1σ limits. Bottom-left panel: reduced χ2 as a function of σadd. Values <1 indicate that modeling the residuals with this much σadd would make the uncertainties inconsistently large compared to the data. Middle column: the probability density distribution (top) and cumulative density (bottom) of the residual spectra, as compared to a normal distribution (black dashed line). A wider distribution here is an indication of unmodeled structure in the residuals. Right column: marginal posterior probability distributions for the additional scatter term σadd. Solid vertical lines show the mean of the distribution, and dashed vertical lines show the ±1σ values. The simple source is best modeled with a very small σadd value (consistent with zero), while the complex source requires a larger value.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse