NIRISS Detector Subarrays
JWST NIRISS detector subarrays are designed to support imaging and spectroscopy observations of targets with a wide range of brightnesses. Smaller subarrays are configured to avoid the risk of saturation and offer high time resolution for bright target observations.
Main article: NIRISS Detector Readout
NIRISS offers four observing modes, including imaging and spectroscopy, that enables a variety of science observations (e.g., exoplanet transits, high redshift galaxies, high resolution imaging of stellar sources, AGNs, etc.). The NIRISS detector is configured for full frame and subarray readout to enable observations of science targets with a wide range in brightnesses.
Full frame readout
In full frame readout, the entire NIRISS detector array is read out through four parallel output channels, each reading a 512 × 2048 pixel region with its own readout amplifier. Full frame readout is the only supported readout for the NIRISS WFSS and NIRSS imaging observing modes.
Main article: NIRISS Bright Limits
NIRISS detector subarrays are read out faster and permit shorter integration times, thereby extending the dynamic range of NIRISS to bright sources. Subarrays also enable observations at high cadence which is particularly useful for science targets that require high time resolution (e.g., exoplanet transits, eclipsing binaries). All subarrays use single channel readout. The subarrays are essential for the NIRISS SOSS and NIRISS AMI modes.
The frame time for a subarray depends on the size of the subarray. The frame times for the SOSS and AMI observing and target acquisition modes are summarized in Tables 1 and 2, respectively. The subarray sizes are given in (x,y) detector coordinates, where x is the slow read direction and y is the fast read direction. Both observing modes can also be observed with full frame readout.
Single object slitless spectroscopy (SOSS)
Table 1. Available NIRISS SOSS subarray modes
2048 × 96
SOSS for bright targets
2048 × 256
SOSS mode default
64 × 64
SOSS target acquisition
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Aperture masking interferometry (AMI)
Table 2. Available NIRISS AMI subarray modes
80 × 80
AMI mode for bright targets
64 × 64
AMI target acquisition