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Table 3
Information summary of the type of exposures acquired during NIRSpec testing, which were then used to extract the different type of reference data necessary for the model optimization.
| Source type (Name) | Slits | GWA | Reference data | Reference type |
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|
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| Continuum (TEST) | MSA all open, FXSL, IFU open | MIRROR | MSA quadrant positions, | Spatial |
| SLIT and IFU positions | ||||
| Continuum (TEST) | MSA checkerboard, FXSL | MIRROR | MSA shutter positions, | Spatial |
| SLIT positions | ||||
| Continuum (FLAT1, 2, 3) | 4 MSA dashed-slit patterns, FXSL | All gratings | Spectrum locations | Spatial |
| Continuum (FLAT3) | MSA closed, IFU open | G395H | Spectrum locations | Spatial |
| MSA closed, IFU closed | G395H | Failed open shutter spectra | † | |
| Absorption lines (REF) | FXSL | All gratings | Spectrum locations, | Spatial |
| spectral feature locations | Spectral | |||
| Emission lines (argon) | 4 MSA dashed-slit patterns, FXSL | All gratings | Line positions | Spectral |
| MSA closed, IFU open | G395H | Line positions | Spectral | |
| MSA closed, IFU closed | G395H | Failed open shutter spectra | † | |
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