Synthetic JWST NIRCam Photometry for 800+ Ultracool Dwarfs
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JWST NIRCam photometry for 800+ ultracool dwarfs synthesized using near-IR SpeX prism spectra. This is a supplementary data product to Sanghi et al. (RNAAS, 7, 194). For research that benefits from this compilation, please cite Sanghi et al. (RNAAS, 7, 194), this Zenodo post, and include the following acknowledgment: "This work has benefitted from The UltracoolSheet, maintained by Will Best, Trent Dupuy, Michael Liu, Aniket Sanghi, Rob Siverd, and Zhoujian Zhang, and developed from compilations by Dupuy & Liu (2012, ApJS, 201, 19), Dupuy & Kraus (2013, Science, 341, 1492), Liu et al. (2016, ApJ, 833, 96), Best et al. (2018, ApJS, 234, 1), Best et al. (2021, AJ, 161, 42), Sanghi et al. (2023), and Schneider et al. (2023, AJ, 166, 103)." Contact asanghi@caltech.edu regarding questions.



