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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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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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