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Table 6

Exposure times and S/N obtained for each synthetic specrum of JWST.

Instrument Mode (a) Exposure time S/N
TOI-5720b
MIRI Slit-less Spectroscopy 7003 s 3095.56
NIRSpec G140H/F070LP 7179 s 3906.26
G140H/F100LP 7168 s 3713.27
G235H/F170LP 7170 s 4072.01
G395H/F290LP 7177 s 3693.03
NIRCam F322W2 7221 s 3514.38
F444W 7177 s 2894.01
NIRISS SUBSTRIP256 7211 s 5645.12
TOI-6008 b
MIRI Slit-less Spectroscopy 8370 s 2513.81
NIRSpec G140H/F070LP (b) 8526 s 3744.90
G140H/F100LP 8510 s 4142.91
G235H/F170LP 8534 s 4258.71
G395H/F290LP 8518 s 3555.67
NIRCam F322W2 8635 s 3536.38
F444W 8500 s 2755.55
NIRISS SUBSTRIP96 (c) 8664 s 6833.68
TOI-6086b
MIRI Slit-less Spectroscopy 8222 s 1934.40
NIRSpec G140H/F070LP 8303 s 3115.41
G140H/F100LP 8315 s 3345.80
G235H/F170LP 8350 s 3214.50
G395H/F290LP 8376 s 3037.43
NIRCam F322W2 8431 s 2903.43
F444W 8516 s 2342.96
NIRISS SUBSTRIP256 8386 s 5107.16

Notes. (a)Details of the different modes, resolving power and wavelength can be found at: https://jwst-docs.stsci.edu/ (b)Disperser-filter combinations. We chose combinations that can provide a high resolution power of 2700. G = Grism, F = Filter. (c)Size of the subarray for single-object slitless spectroscopy.

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