NIRISS Imaging Calibration Status
The overall calibration status and estimated accuracy of NIRISS imaging are described in this article; please also see the article on known issues affecting NIRISS imaging data.
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Astrometric accuracy
Date:
Relative astrometric accuracy within the detector is about 3 mas (rms, single axis). Absolute astrometric accuracy for observations without target acquisition (TA) is typically less than 0.1 arcsec (single axis), while for observations with TA, the accuracy is about 2 mas (rms, single axis). Note that in rare cases (e.g., crowded fields, high background, etc), the telescope can inadvertently guide on a star that is offset from the commanded location, and this can lead to the world coordinate system (WCS) of the observed image being offset by 1–2 arcsec or more.
Photometric calibration
Updated:
As of CRDS context jwst_1296.pmap, the scaling factors in the imaging photometry reference files (to convert count rates from units of ADU/S to MJy/ster) have accuracies raning from 0.06 - 0.42% (see Volk and Goudfrooij 2025).
Filter-to-filter image offsets (i.e., boresight offsets)
Date:
Words in bold are GUI menus/
panels or data software packages;
bold italics are buttons in GUI
tools or package parameters.
Table 1. Filter-to-filter offsets in NIRISS "rate.fits" and "cal.fits" images
| Filter | x pixel offset | y pixel offset |
|---|---|---|
| F090W | -0.1529 | +0.7676 |
| F115W | +0.0397 | -0.0651 |
| F140M | +0.0173 | +0.0650 |
| F150W | 0.0 | 0.0 |
| F158M | -0.4397 | -0.1929 |
| F200W | +2.1190 | -1.0476 |
| F277W | +0.2213 | -0.1309 |
| F356W | +0.0429 | -0.2291 |
| F380M | -0.2747 | +0.3512 |
| F430M | +0.0346 | -0.0113 |
| F444W | +0.1658 | -0.1387 |
| F480M | -0.2197 | +0.1298 |
References
Volk, K., and Goudfrooij, P., 2025, AJ, 170, 136
The James Webb Space Telescope Absolute Flux Calibration. IV. Near-Infrared Imager and Slitless Spectrograph Imaging