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Stochastic Optical Variability and an rms–Flux Relation in the Intermediate Polar EP240309a

  • Authors: S.-Y. Wu, Y.-D. Hu, I. Pérez-García, A. J. Castro-Tirado, M. Gritsevich, E. J. Fernández-García, M. D. Caballero-García, S. Guziy, G. García-Segura, R. Sánchez-Ramírez, C. D. Kilpatrick, C. R. Bom, L. Santana, A. Santos, P. J. Meintjes, H. J. van Heerden, A. Martín-Carrillo, L. Hanlon, A. Maury, D.-R. Xiong, B.-B. Zhang

S.-Y. Wu et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 4.

Example Gaussian + linear-baseline fits to six prominent emission lines used to estimate centroids and deconvolved widths. We annotate the fitted centroid λc and the corresponding apparent velocity offset vγ = c(λc/λ0 − 1) in each panel; the annotated vFWHM values are derived from deconvolved widths (see Section 3.5).

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