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
{"title":"A Systematic Search for Galaxies with Extended Emission Line and Potential Outflows in JADES Medium-Band Images","authors":"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","doi":"arxiv-2409.11464","DOIUrl":null,"url":null,"abstract":"For the first time, we systematically search for galaxies with extended\nemission line and potential outflows features using medium-band images in the\nGOODS-S field by comparing the morphology in medium-band images to adjacent\ncontinuum and UV bands. We look for galaxies that have a maximum extent 50\\%\nlarger, an excess area 30\\% greater, or an axis ratio difference of more than\n0.3 in the medium band compared to the reference bands. After visual\ninspection, we find 326 candidate galaxies at $1 < z < 6$, with a peak in the\npopulation near cosmic noon, benefiting from the good coverage of the\nmedium-band filters. By examining their SEDs, we find that the candidate\ngalaxies are at least 20\\% more bursty in their star-forming activity and have\n60\\% more young stellar populations compared to a control sample selected based\non the continuum band flux. Additionally, these candidates exhibit a\nsignificantly higher production rate of ionizing photons. We further find that\ncandidates hosting known AGN produce extended emission that is more anisotropic\ncompared to non-AGN candidates. A few of our candidates have been\nspectroscopically confirmed to have prominent outflow signatures through\nNIRSpec observations, showcasing the robustness of the photometric selection.\nFuture spectroscopic follow-up will better help verify and characterize the\nkinematics and chemical properties of these systems.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"52 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11464","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
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.