Spectra From Precise Bolometric Luminosities and Effective Temperatures of 23 late-T and Y dwarfs Obtained with JWST
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This archive contains the data behind Figures 5-7 of the published version of the manuscript listed above (Beiler et al. 2024b, https://doi.org/10.3847/1538-4357/ad6301). These data include the merged JWST NIRSpec and MIRI LRS. The full reduction, marging, and calibration process can be found in Section 4. For any questions, contact Samuel Beiler <Samuel.Beiler@rockets.utoledo.edu>.
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Zenodo创建时间：
2025-03-05
