An early contender for observation time, the "Next Generation Deep Extragalactic Exploratory Public" will build on Hubble's deep field observations. The "P.I." is a Hubble Fellow with plenty of experience in Deep Field, high redshift work.
From the news release:
https://webbtelescope.org/contents/news-releases/2022/news-2022-015.html
(“We’re using two science instruments at once, and they will observe continuously.” They will point Webb’s Near-Infrared Imager and Slitless Spectrograph (NIRISS) on the primary Hubble Ultra Deep Field, and Webb’s Near-Infrared Camera (NIRCam) on the parallel field, getting twice the bang for their “buck” of telescope time.)
Principal Investigator, Prof. S. Finkelstein
NGDEEP Proposal #2079 Cycle: 1, GO
https://www.stsci.edu/jwst/phase2-public/2079.pdf
An overview from the above pdf.
"We propose NGDEEP: The Webb Deep Extragalactic Exploratory Public Survey. NGDEEP leverages efficient parallel observations over 121.7 hr with NIRISS in the Hubble Ultra Deep Field (HUDF) and NIRCam in the HUDF-Par2 field to constrain the physical processes dominating feedback in galaxies from z~1-12. Observing with JWST in the HUDFs leverages off the deepest optical imaging from Hubble and makes NGDEEP a premier legacy field for both missions.
NGDEEP observes deeply with NIRISS (60-190 ks) to detect faint emission lines (~ 10^-18 cgs) for >1000 mostly low-mass (log M/Msol = 7-9) galaxies. NGDEEP-NIRISS will enable robust constraints on the low-mass end of the mass-metallicity relation and constrain stochastic star-formation by probing H-alpha based star-formation rates to 0.1 Msol/yr in these low-mass galaxies. These measurements will limit chemical enrichment and feedback physical prescriptions in models, which are currently unconstrained at these masses.
In parallel, NGDEEP will obtain the deepest 6-band NIRCam imaging (m~30.6-30.9) on the HUDF-Par2 field. NGDEEP-NIRCam will probe z > 12, and constrain stellar feedback prescriptions in models by precisely measuring the shape of the faint-end of the UV luminosity function at z~10. These data will provide unprecedented morphological detail in galaxies at all redshifts, and reconnoiter the sites of first black hole formation.
Being public immediately, NGDEEP follows in the footsteps of the Hubble deep field programs, enabling the community to explore the power of Webb when pushed to its limits. As a treasury program, we are committed to the rapid reduction and release of high-quality reduced data products and catalogs."