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Table 1

Parameters used to compute the expected spectral precision on the transit and eclipse depth of TOI-519 b using NIRISS-SOSS, NIRSpec-PRISM, or MIRI-LRS.

Instrument Groups per integration Exposure time (s) Precision white light curve (ppm/min)
NIRISS- SOSS 84 466 34
NIRSpec- PRISM 6 1.6 190
MIRI-LRS 469 74.7 1272

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