Fig. 5
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Average number of spectra 
that can be accommodated on the NIRSpec detector array in MOS mode without overlap as a function of nvs, the number of candidate targets located within Viable Slitlets on the MSA. The points show the results of 10 000 Monte Carlo trials carried out at the shown values of nvs for the PRISM and the G235M grating. The continuous curves show the fits to Eq. (5).
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