Context. The physical properties of almost any kind of astronomical object can be derived by fitting synthetic spectra or photometry extracted from theoretical models to observational data.

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Bayo et al. (Thu,) studied this question.

synapsesocial.com/papers/6a1bf03126cb5670aa9d22eb https://doi.org/https://doi.org/10.1051/0004-6361:200810395

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Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1An Effective Temperature Scale for Late‐M and L Dwarfs, from Resonance Absorption Lines of Cs<scp>i</scp>and Rb<scp>i</scp>2000 · 244 citations
2The Infrared Array Camera (IRAC) for the <i>Spitzer Space Telescope</i>2004 · 3,387 citations
3The Two Micron All Sky Survey (2MASS)2006 · 12,145 citations
4Estimating stellar parameters from spectra2004 · 13 citations
5Discovery of optically faint obscured quasars with Virtual Observatory tools2004 · 40 citations