Synthetic JWST NIRCam, Euclid NISP, and Roman WFI Near-Infrared Photometry for 800+ Ultracool Dwarfs
Creators
- 1. Department of Astronomy, California Institute of Technology, 1200 E. California Boulevard, Pasadena, CA 91125, USA
- 2. Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
- 3. The University of Texas at Austin, Department of Astronomy, 2515 Speedway, C1400, Austin, TX 78712, USA
- 4. Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK
- 5. University of California, Santa Cruz, 1156 High St. Santa Cruz, CA 95064, USA
Description
JWST NIRCam, Euclid NISP, and Roman WFI photometry (apparent magnitudes) for 800+ ultracool dwarfs synthesized using near-IR SpeX prism spectra. This is a supplementary data product to Sanghi et al. 2023 (RNAAS, 7, 194) and Sanghi et al. 2024 (RNAAS, 8, 137). JWST photometry is presented in the Vega magnitude system and Euclid and Roman photometry are presented in the AB magnitude system.
For research that benefits from this compilation, please cite Sanghi et al. 2023 (RNAAS, 7, 194) for JWST photometry, Sanghi et al. 2024 (RNAAS, 8, 137) for Euclid and Roman photometry, 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, ApJ, 959, 63), and Schneider et al. (2023, AJ, 166, 103)."
Contact asanghi@caltech.edu regarding questions.
Notes
Version 2.0.0: Adds synthetic photometry in the Euclid and Roman Space Telescope near-infrared filters (AB magnitude system).
Files
JWST-Euclid-Roman-synth-phot.csv
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Additional details
Related works
- Is published in
- Journal article: 10.3847/2515-5172/acf864 (DOI)