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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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