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VLITE Observations of the Hubble Ultra Deep Field

We present 136 hr of 340 MHz observations of the Hubble Ultra Deep Field (HUDF) conducted with the VLA Low-band Ionosphere and Transient Experiment (VLITE), collected commensally with higher-frequency Karl G.

By Polisensky, Peters, Giacintucci +3

Score█████░░░░░4.6

Key numbers

  • 30% likely require an intrinsic
  • 5 sigma significance

VerdictWorth a reader's time today.

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Abstract

We present 136 hr of 340 MHz observations of the Hubble Ultra Deep Field (HUDF) conducted with the VLA Low-band Ionosphere and Transient Experiment (VLITE), collected commensally with higher-frequency Karl G. Jansky Very Large Array (VLA) observations. Our deepest image combines 20 hr of data, covers 4 square degrees, and achieves an angular resolution of 8.8 arcsec x 3.8 arcsec with an rms sensitivity of 158 microJy per beam at the field center. We catalog 671 radio sources detected above 5 sigma significance. Correcting for incompleteness using injection-recovery simulations with a model radio continuum population, we show that our source counts recover the sub-mJy star-forming galaxy population at abundances consistent with other deep fields at comparable frequencies. The data span 45 observing days across two VLA A-configuration semesters separated by 1.3 years, providing a search for variability on ~1-year timescales at sub-mJy flux densities. We identify eleven variable sources with flux densities of 1-100 mJy and modulation indices of 6-40%, six of which exhibit peaked radio spectra consistent with compact AGN. Their variability amplitudes are consistent with refractive interstellar scintillation (RISS) predicted for this line of sight, though three sources with modulation indices exceeding 30% likely require an intrinsic contribution. One source, subsequently confirmed as a compact symmetric object through VLBA follow-up observations, demonstrates the potential of VLITE for identifying populations of young radio AGN through commensal low-frequency variability searches.

Emil Polisensky, Wendy Peters, Simona Giacintucci, Kristina Nyland, Tracy Clarke, Amaris McCarver

The editor's rubric

Heuristic review

Leverage3 / 5
A method or resource many groups across the field will adopt within a year.
18% of this desk’s rubric
Magnitude3 / 5
Large gain: roughly 2x, or a clear new state of the art on a hard, unsaturated problem.
20% of this desk’s rubric
Evidence4 / 5
Strong: large scale, preregistered, independently replicated, or a well-powered randomized trial.
22% of this desk’s rubric
Novelty3 / 5
A genuinely new approach to an open problem.
22% of this desk’s rubric
Trajectory2 / 5
Some room to improve with obvious engineering.
10% of this desk’s rubric
Stakes2 / 5
Benefits a professional community (practitioners, clinicians, engineers).
8% of this desk’s rubric

Editor’s rationale

Heuristic triage from title and abstract text only, not a reading of the paper. Cues found: method (we propose, we report); gains (outperforms); novelty (open problem, discovery); verification (sigma, independent replication).

How the score was computed

rank-2026-10-18

Score█████░░░░░4.6

Score = 10 × (75% × adjusted merit / 10 + 15% × attention + 10% × freshness)

Desks place stronger verdicts first, then use this score to order work within the same verdict.

Merit
6.1 / 10
Weighted rubric, evidence-gated.
Adjusted merit
4.9 / 10
Shrunk toward the desk prior by editor confidence (44%).
Attention
0%
Citations, upvotes, points, mentions.
Freshness
95%
Half-life decay since publication.

No attention signals recorded yet.

The record

  • Reviewed by heuristic-v10 on Nov 3, 2026, 07:29 UTC. Paper type: method.
  • Categories: astro-ph.GA
  • TOP, No.2 in the Front page edition of November 3, 2026.
  • LEAD, No.1 in the Physics edition of November 3, 2026.