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The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744

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arxiv 2408.03920 v3 pith:DY722XNY submitted 2024-08-07 astro-ph.GA

classification astro-ph.GA
keywords galaxiesjwstmathrmnirspecabellclusternircamobserved
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abstract

We present the design and observations of low resolution JWST/NIRSpec PRISM spectroscopy from the Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program. Targets are selected using JWST/NIRCam photometry from UNCOVER and other programs, and cover a wide range of categories and redshifts to ensure the legacy value of the survey. These categories include the first galaxies at $z\gtrsim10$, faint galaxies during the Epoch of Reionization ($z\sim6-8$), high redshift AGN ($z\gtrsim6$), Population III star candidates, distant quiescent and dusty galaxies ($1\lesssim{}z\lesssim 6$), and filler galaxies sampling redshift--color--magnitude space from z~0.1-13. Seven NIRSpec MSA masks across the extended Abell 2744 cluster were observed, along with NIRCam parallel imaging in 8 filters (F090W, F115W, F150W, F200W, F277W, F356W, F410M, F444W, F480M) over a total area of ~26 arcmin$^2$, overlapping existing HST coverage from programs including the Hubble Frontier Fields and BUFFALO. We successfully observed 553 objects down to $m_{\mathrm{F444W}}\sim30\mathrm{AB}$, and by leveraging mask overlaps, we reach total on-target exposure times ranging from 2.4-16.7h. We demonstrate the success rate and distribution of confirmed redshifts, and also highlight the rich information revealed by these ultradeep spectra for a subset of our targets. An updated lens model of Abell 2744 is also presented, including 14 additional spectroscopic redshifts and finding a total cluster mass of $M_{\mathrm{SL}}=(2.1\pm0.3)\times10^{15}\,\mathrm{M}_{\odot}$. We publicly release reduced 1D and 2D spectra for all objects observed in Summer 2023 along with a spectroscopic redshift catalog and the updated lens model of the cluster (https://jwst-uncover.github.io/DR4.html).

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Forward citations

Cited by 7 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

    astro-ph.GA 2025-09 conditional novelty 7.0 of 10

    Directly integrating the observed spectra of two Little Red Dots shows the bolometric luminosity is dominated by rest-frame optical light, lowering implied black hole masses to about 10^5 to 10^7 solar masses.

  2. The Impact of Galaxy Overdensities and Ionized Bubbles on Ly$\alpha$ Emission at $z\sim7.0-8.5$

    astro-ph.GA 2025-05 conditional novelty 7.0 of 10

    Strong Lyα emitters at z~7-8.5 are preferentially found in galaxy overdensities comparable in size to predicted ionized bubbles, with the EGS field showing evidence for an unusually large ionized sightline.

  3. A Massive Galaxy at the Edge of Feedback-Free Efficiency

    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    UNCOVER 3686 at z = 9.31 has a star-formation efficiency of 20–60%, 2–6 times above empirical models and consistent with the feedback-free starburst scenario.

  4. ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs

    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    Balmer-line absorption occurs in ~35% (14/40) of JWST little-red-dot AGNs, roughly 850x the rate in SDSS type-1 AGNs, with mostly slow blueshifted absorber velocities.

  5. Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution

    astro-ph.GA 2026-06 unverdicted novelty 6.0 of 10

    LRDs transition from underdense low-halo-mass environments at z>4 to typical galaxy conditions by z~3.5, with halo growth leading to larger sizes and SED changes that explain their disappearance at lower redshifts.

  6. The impact of medium-width bands on the selection, and subsequent luminosity function measurements, of high-z galaxies

    astro-ph.GA 2025-02 conditional novelty 6.0 of 10

    Using the JADES Origins Field, the authors show that medium-band photometry modestly improves high-z galaxy selection completeness, while bluer broadband depth matters most for reducing contamination.

  7. Probing Obscured Star Formation in Galaxy Clusters Using JWST Medium Band Images: 3.3$\mu\rm m$ PAH Emitter Sample in Abell 2744

    astro-ph.GA 2025-06 conditional novelty 5.0 of 10

    JWST F430M medium-band imaging isolates 3.3 micron PAH emission and identifies 22 star-forming galaxies in Abell 2744 whose PAH-based star formation rates match SED and far-infrared estimates, placing them mostly in l...

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