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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 17.

Keplerian model of ﹩{v}_{\star }^{{\mathtt{SSOF}}}﹩. Left: ﹩{v}_{\star }^{{\mathtt{SSOF}}}﹩ after phase folding at the planet period (blue) and the MAP Keplerian RVs (orange). Center: ﹩{v}_{\star }^{{\mathtt{SSOF}}}-﹩ MAP Keplerian RVs residuals (blue). Much more remains in the residuals than can be adequately explained by the measurement noise alone.

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