Table 11
Forthcoming space observations of Gl 486 and Gl 486 b in the optical and infrared.
Program | Telescope | Instrument | Mode | ∆λ(a) | R (λ/∆λ) | Visit time (h) | Remark |
---|---|---|---|---|---|---|---|
Sector50 | TESS | Camera 1 | 2 min cadence | 6000–10000Å | ~2 | ~650 | Photometry |
GO 1743 | Webb | MIRI | LRS slitless prism | 5–12 µm | ~100 | 2 × 6.27 | Secondary eclipse |
GO 1981 | Webb | NIRSpec | BOTS G395H/F290LP | 2.87–5.18 µm | 1900–3700 | 2 × 5.14 | Transmission spectra |
GO 16722 | Hubble | COS | NUV/G230L | 1700–3200Å | 2100–3200 | 0.15 | |
COS | FUV/G160M | 1405–1775Å | 13 000–24000 | 1.88 | |||
COS | FUV/G130M | 900–1236Å | <11 500 | 2.11 | |||
STIS | FUV/G140M | 1140–1740Å | 11 400-17 400 | 1.36 | Lyα |
Notes. Scheduled TESS observations in Year 4+ from 25 March 2022 to 22 April 2022 accessed from https://heasarc.gsfc.nasa.gov/cgi-bin/tess/webtess/wtv.py?Entry=gj+486. Accepted Webb general observer cycle 1 (2nd half 2022-1st half 2023) programmes accessed from https://www.stsci.edu/jwst/science-execution/approved-programs/cycle-1-go. Accepted Hubble general observer cycle 29 (1 October 2021-30 September 2022) programmes accessed from https://www.stsci.edu/hst/proposing/approved-programs. Joint Hubble and XMM-Newton programme GO 16722 accessed from https://archive.stsci.edu/hst/joint_programs.html. (a)For the sake of readability, we mix wavelength units.
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