A Systematic Search for Galaxies with Extended Emission Lines and Potential Outflows in JADES Medium-band Images

  • Yongda Zhu
  • , Marcia J. Rieke
  • , Zhiyuan Ji
  • , Charlotte Simmonds
  • , Fengwu Sun
  • , Yang Sun
  • , Stacey Alberts
  • , Rachana Bhatawdekar
  • , Andrew J. Bunker
  • , Phillip A. Cargile
  • , Stefano Carniani
  • , Anna de Graaff
  • , Kevin Hainline
  • , Jakob M. Helton
  • , Gareth C. Jones
  • , Jianwei Lyu
  • , George H. Rieke
  • , Pierluigi Rinaldi
  • , Brant Robertson
  • , Jan Scholtz
  • Hannah Übler, Christina C. Williams, Christopher N.A. Willmer

Research output: Contribution to journalArticlepeer-review

Abstract

For the first time, we present a systematic search for galaxies with extended emission lines and potential outflow features using JWST medium-band images in the GOODS South field. This is done by comparing the morphology in medium-band images to adjacent continuum and UV bands. We look for galaxies that have a maximum extent 50% larger, an excess area 30% greater, or an axis ratio difference of more than 0.3 in the medium band compared to the reference bands. After visual inspection, we find 326 candidate galaxies at 1.4 < z < 8.4, with a peak in the population near cosmic noon, benefiting from the good coverage of the medium-band filters. By fitting their spectral energy distributions, we find that the candidate galaxies are at least 20% more bursty in their star-forming activity and have 50% more young stellar populations compared to a control sample selected based on the continuum band flux. Additionally, these candidates exhibit a significantly higher production rate of ionizing photons. We further find that candidates hosting known active galactic nuclei (AGN) produce extended emission that is more anisotropic compared to non-AGN candidates. A few of our candidates have been spectroscopically confirmed to have prominent outflow signatures through NIRSpec observations, showcasing the robustness of the photometric selection. Future spectroscopic follow-up will better help verify and characterize the kinematics and chemical properties of these systems.

Original languageEnglish (US)
Article number162
JournalAstrophysical Journal
Volume986
Issue number2
DOIs
StatePublished - Jun 20 2025

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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