New NIRSpec BOTS Prism Multistripe Capability To Observe Brighter Targets

August 19, 2026

About This Article

In Cycle 6, NIRSpec is offering the new ‘multistripe’ readout capability for BOTS Prism observations. This method dramatically reduces frame time and increases the bright-source limit, allowing observations of brighter sources over a broad (0.6-5 microns) wavelength range. BOTS multistripe subarrays can only be used with the PRISM/CLEAR disperser-filter combination. For the smallest multistripe subarray, the new 2-group bright limit is J ~ 8 and the frame times are ~15x shorter compared to the nominal Prism SUB512 subarray. These gains come at the expense of reduced exposure efficiency, as only a portion of the subarray is read out at any given time. Instead of reading a single subarray region, the multistripe subarrays split the subarray into multiple regions (or “stripes”) that are read out individually, with the stripe moving to a different location in the subarray after the integration for the previous stripe is completed (Figure 1).

On August 20th, JWebbinar 52 – Developments in Instrument Modes and Capabilities for JWST Cycle 6 will cover the details of this new capability. Observers are encouraged to attend the JWebbinar and to contact the NIRSpec team through the JWST Help Desk with any questions.

nirspec-readout-news.jpg
Figure 1: Depiction of a BOTS prism multistripe observation. Within the SUB512 footprint, portions of the NRS1 detector ("stripes") are read out as sub-integrations (blue) that step through the Prism region in wavelength space (top). The top panel shows 4 stripes, as used by the SUB128M4_PRISM subarray. In the time-series readout (bottom), 4 reference pixels (orange) are interleaved at the start of each sub-integration for calibration purposes.  

 

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.