New Pathloss Corrections for NIRSpec Multi-Object and Fixed Slit Spectroscopy Are Available

November 11, 2025

About This Article

JWST Pipeline Build 12.1, currently available to users and planned for operations later in the year, includes improved pathloss correction reference files for the NIRSpec Multi-Object Spectroscopy (MOS) and Fixed Slit (FS) observing modes. The new pathloss corrections are based on in-flight data.

Pathloss is the flux lost outside an aperture and depends on wavelength, target type, and the position within the shutter/slit. This update assumes two target cases: compact point sources or sources uniformly extended throughout the shutter/slit.

Point Source Updates (MOS only): The relative flux calibration accuracy is improved from ~8% to ~5% for well-centered targets and from as high as ~70% to ~10-15% for targets near the MSA shutter edges. See Figure 1 Top panel. 

Uniform Source Updates: Now yield consistent background measurements to within ~5% across all MOS and FS apertures. These measurements also more closely match predictions from the JWST Background Tool (JBT) model. See Figure 1 Bottom panel.

Users with questions about the new pathloss corrections are encouraged to contact the NIRSpec team via the Help Desk.

pathloss-news.jpg
Figure 1: Build 12.0 (left) vs. Build 12.1 (right). Top: Example point source MOS PRISM spectra from PID 1133, including two well-centered sources and a few near the shutter edge, as shown in the inset. The plots show differences relative to the centered spectrum. Bottom: Example sky background (uniform) PRISM spectra from PID 2750 extracted from empty MOS shutters and each FS, along with the JBT model prediction at the time of observation (known to be less accurate below ~1.2 µm). The plots show differences relative to the S1600A1 reference spectrum.

 

Share This Page

This site is protected by reCAPTCHA and the Google

Webb Space Telescope insignia

 

For technical assistance, please contact the JWST Help Desk.

 

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