Pipeline News: Build 12.1 of the Science Calibration Pipeline Is Now Available
Build 12.1 includes improvements to all four JWST instruments.

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Build 12.1 includes improvements to all four JWST instruments.

Cycle 5 proposals can take advantage of NIRCam and NIRISS multistripe capabilities.

These new images significantly improve the subtraction of the sky background in WFSS data.

Build 12.0 includes improvements for MIRI, NIRCam, and NIRISS as well as time-series observations.

Build 10.2 includes several upgrades for the NIRISS Aperture Masking Interferometry (AMI) mode.

JWST's NIRISS instrument has resumed observations.

Tests are being conducted and a number of pure parallel observations are being executed to determine the cause.

JWST observers can now use Mirage to produce realistic NIRCam and NIRISS simulated data to help them understand and prepare for JWST before launch.

The Aperture Masking Interferometry (AMI) mode of JWST’s Near Infrared Imager and Slitless Spectrograph (NIRISS) offers a unique capability of high-resolution, moderate contract imaging at small separations.

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The NASA James Webb Space Telescope, developed in partnership with ESA and CSA, is operated by AURA’s Space Telescope Science Institute.