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Data-driven Modeling of Telluric Features and Stellar Variability with StellarSpectraObservationFitting.jl

  • Authors: Christian Gilbertson, Eric B. Ford, Samuel Halverson, Evan Fitzmaurice, Cullen H. Blake, Gumundur Stefánsson, Suvrath Mahadevan, Jason T. Wright, Jacob K. Luhn, Joe P. Ninan, Paul Robertson, Arpita Roy, Christian Schwab, Ryan C. Terrien

Christian Gilbertson et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 12.

Lomb–Scargle periodogram of ﹩{v}_{\star }^{{\mathtt{SSOF}}}﹩ for HD 26965. The period of the maximum peak is labeled. The horizontal lines are the 95%, 97.72% (one-sided 2σ), 99%, and 99.87% (one-sided 3σ) false alarm probability powers based on the distribution of maximum powers from many Lomb–Scargle periodograms of bootstrap reorderings of ﹩{v}_{\star }^{{\mathtt{SSOF}}}﹩. The dominant signal remaining is very significant and at the stellar rotation period.

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