A Systematic Search for Galaxies with Extended Emission Line 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
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Abstract

For the first time, we systematically search for galaxies with extended emission line and potential outflows features using medium-band images in the GOODS-S field 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 $1 < z < 6$, with a peak in the population near cosmic noon, benefiting from the good coverage of the medium-band filters. By examining their SEDs, we find that the candidate galaxies are at least 20\% more bursty in their star-forming activity and have 60\% 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 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.
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在 JADES 中波段图像中系统搜索具有扩展发射线和潜在外流的星系
通过比较中波段图像与邻近连续波段和紫外波段图像的形态,我们首次利用GOODS-S场的中波段图像系统地搜索了具有扩展发射线和潜在外流特征的星系。我们寻找在中波段与参考波段相比,最大范围大50%,过剩面积大30%,或者轴比差异超过0.3的星系。经过目视检查,我们发现了326个候选星系,它们的年龄在1<z<6元,在宇宙正午附近的星系数量达到了一个峰值,这得益于中波段滤光片的良好覆盖。通过研究它们的SED,我们发现与根据连续波段通量选取的对照样本相比,候选星系的恒星形成活动至少多了20%,年轻恒星群多了60%。此外,这些候选星的电离光子产生率明显更高。我们还发现,与非AGN候选星相比,寄存在已知AGN中的候选星产生的扩展辐射更具各向异性。通过近红外望远镜的观测,我们的一些候选者被光谱学证实具有突出的外流特征,这展示了光度选择的稳健性。未来的光谱学跟踪将更好地帮助验证和描述这些系统的动力学和化学性质。
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