Image Details

Choose export citation format:

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 2.

Flowchart for the SSOF model searching process up to (K⊕ ≤ 1, K⋆ ≤ 1) model components. Each hexagonal cell indicates the comparison of two different proposed SSOF models. Starting from the basic SSOF(﹩\varnothing ﹩,0) model (with no telluric template or feature vectors and no stellar feature vectors), we repeatedly check whether adding a telluric or stellar model component is “better” (which in our case we take to be the one with a lower AIC) and add the corresponding component until we reach the desired final model complexity. SSOF(﹩\varnothing ﹩,1), SSOF(0,1), and SSOF(1,0) lead directly to one other SSOF model because they are already at one of the specified feature vectors limits. Once the search is completed up to SSOF(K⊕, K⋆), the best SSOF model found along the searched path is used for further analyses. The flowchart defines a deterministic procedure, leaving no free choices for the user.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse