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Table 5
Wavelength coverage and resolving power (R) of the instruments on JWST and ELT used to calculate the number of transits required to detect spectral features in the atmosphere of LHS 1140 b.
| Telescope - Instrument | Wavelength | R | Ref. |
|---|---|---|---|
| JWST - NIRSpec PRISM | 0.6–5.3 μm | ~100 | (1) |
| JWST - MIRI LRS | 5.0–12 μm | ~100 | (2) |
| ELT - HIRES | 0.37–2.5 μm | 100 000 | (3) |
| ELT - METIS (HRS) | 2.9–5.3 μm | 100 000 | (4) |
References. (1) Birkmann et al. (2016); (2) Kendrew et al. (2015); (3) Marconi et al. (2016); (4) Brandl et al. (2016).
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