Rocky Worlds DDT Information Session Coming Soon
The January 21, 2025 information session will include team updates, first observations, and data products.
The January 21, 2025 information session will include team updates, first observations, and data products.
Reminder: Please take the survey before it closes on December 23, 2024.
Build 11.1 of the JWST Science Calibration Pipeline provides major improvements for multiple observing modes
Help us improve the JWST user experience by taking the survey.
The astronomical community will have many opportunities to participate in JWST-related workshops and special sessions during the upcoming 245th AAS meeting.
The latest JSTUC meeting included presentations on a variety of topics, such as Cycle 4 submission statistics, new initiatives for Cycle 5, plans for future community outreach, and various working group updates.
JWST users can access archived wavefront maps and utilize STScI tools to visualize and trend JWST wavefront errors to better understand JWST image quality.
STScI received a total of 2,377 proposals, requesting ~78,000 hours of observing time for the Cycle 4 Call for Proposals.
STScI’s JWST Science Calibration Pipeline now uses quarterly fixed reference file contexts to process and reprocess data.
Proposers facing extenuating circumstances may contact the Help Desk to request a moderate extension.
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.
Director's Discretionary (DD) time proposals to support observations of compelling scientific urgency are now available.
An initial set of targets for MIRI 15 µm photometry has been identified.
There are significant changes affecting proposal preparation this cycle.
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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.