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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 2.

Full-night BOOTES PSD (fractional rms² Hz⁻¹) for the longest sequence, with the adopted analysis band and best-fitting SPL/BPL continua overplotted. The SPL continuum is mildly preferred over the BPL and TK simulations do not reject the SPL null hypothesis, so no bend is claimed within the sampled frequency range.

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