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.

This new mode enables efficient spectroscopic observations of multiple sources in a single pointing.

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

New models of the count rate better predict the decrease in future observing cycles. These models will be incorporated into upcoming Build 12.1 of the pipeline (expected November 2025) and Cycle 6 of the JWST ETC.

Build 11.3 includes an improved algorithm to correct for MIRI MRS cosmic ray showers in faint sources.

New and improved calibrations are now available for both the MIRI Low-Resolution Spectrometer (LRS) fixed-slit and slitless modes.

The photometric calibration reference files for the Medium Resolution Spectrometer have been updated to reflect a more comprehensive analysis using data obtained over the course of JWST Cycles 1 and 2.

A zero exclusive access period now applies to data from MIRI observations of coronagraphic PSF reference star-associated background targets.

The improved correction is available in the latest version of the JWST Calibration Pipeline and replaces the correction provided in September 2023.

New reference files for the MIRI Low-Resolution Spectrometer (LRS) improve the wavelength and photometric calibration, as well as the aperture correction.

Investigations over the last 18 months help characterize the decline in the MIRI count rate.

As a result of continued analysis of calibration observations and improvements in code and algorithms, significant updates to the Imaging and Coronagraphic Imaging flux calibration reference files are now available.

Calibration data reveals a reduced count rate in the long-wavelength filters of the MIRI Imager.

Multiple updates to the MIRI Medium Resolution Spectrometer (MRS) pipeline and the associated reference files are now available.

This update reports on a careful study of the impact the measured MIRI MRS decrease count rate has on science data, as well as on the upcoming pipeline mitigation.

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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.