Discovery of extreme [O III]+Hβ emitting galaxies tracing an overdensity at z ∼ 3.5 in CDF-South

Ben Forrest, Kim-Vy H. Tran, Adam Broussard, Rebecca J. Allen, Miranda Apfel, Michael J. Cowley, Karl Glazebrook, Glenn G. Kacprzak, Ivo Labbé, Themiya Nanayakkara, Casey Papovich, Ryan F. Quadri, Lee R. Spitler, Caroline M. S. Straatman, Adam Tomczak

    Research output: Contribution to journalArticlepeer-review

    40 Citations (Scopus)

    Abstract

    Using deep multi-wavelength photometry of galaxies from zfourge, we group galaxies at 2.5 < z < 4.0 by the shape of their spectral energy distributions (SEDs). We identify a population of galaxies with excess emission in the K s-band, which corresponds to [O III]+Hβ emission at 2.95 < z < 3.65. This population includes 78% of the bluest galaxies with UV slopes steeper than β = -2. We de-redshift and scale this photometry to build two composite SEDs, enabling us to measure equivalent widths of these extreme [O III]+Hβ emission line galaxies (EELGs) at z ∼ 3.5. We identify 60 galaxies that comprise a composite SED with a [O III]+Hβ rest-frame equivalent width of 803 ±228 Å and another 218 galaxies in a composite SED with an equivalent width of 230 ±90 Å. These EELGs are analogous to the "green peas" found in the SDSS and are thought to be undergoing their first burst of star formation due to their blue colors (β < -1.6), young ages (log(age yr-1) ∼ 7.2), and low dust attenuation values. Their strong nebular emission lines and compact sizes (typically ∼1.4 kpc) are consistent with the properties of the star-forming galaxies possibly responsible for reionizing the universe at z > 6. Many of the EELGs also exhibit Lyα emission. Additionally, we find that many of these sources are clustered in an overdensity in the Chandra Deep Field South, with five spectroscopically confirmed members at z = 3.474 ± 0.004. The spatial distribution and photometric redshifts of the zfourge population further confirm the overdensity highlighted by the EELGs.

    Original languageEnglish
    Article numberL12
    Pages (from-to)1-6
    Number of pages6
    JournalAstrophysical Journal Letters
    Volume838
    Issue number1
    DOIs
    Publication statusPublished - 20 Mar 2017

    Keywords

    • galaxies: evolution
    • galaxies: formation
    • galaxies: high-redshift
    • galaxies: starburst
    • large-scale structure of universe
    • ultraviolet: galaxies

    Fingerprint

    Dive into the research topics of 'Discovery of extreme [O III]+Hβ emitting galaxies tracing an overdensity at z ∼ 3.5 in CDF-South'. Together they form a unique fingerprint.

    Cite this