The size evolution of star-forming galaxies since z ∼ 7 using ZFOURGE

Rebecca J. Allen, Glenn G. Kacprzak, Karl Glazebrook, Ivo Labbé, Kim-Vy H Tran, Lee R. Spitler, Michael Cowley, Themiya Nanayakkara, Casey Papovich, Ryan Quadri, Caroline M S Straatman, Vithal Tilvi, Pieter Van Dokkum

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    62 Citations (Scopus)
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    Abstract

    For the first time, we present the size evolution of a mass-complete (log(M /M o) > 10) sample of star-forming galaxies over redshifts z = 1-7, selected from the FourStar Galaxy Evolution Survey. Observed H-band sizes are measured from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) Hubble Space Telescope (HST)/F160W imaging. Distributions of individual galaxy masses and sizes illustrate that a clear mass-size relation exists up to z ∼ 7. At z ∼ 7, we find that the average galaxy size from the mass-size relation is more compact at a fixed mass of log(M /M o) = 10.1, with kpc, than at lower redshifts. This is consistent with our results from stacking the same CANDELS HST/F160W imaging, when we correct for galaxy position angle alignment. We find that the size evolution of star-forming galaxies is well fit by a power law of the form kpc, which is consistent with previous works for normal star-formers at 1 < z < 4. In order to compare our slope with those derived Lyman break galaxy studies, we correct for different IMFs and methodology and find a slope of -0.97 ± 0.02, which is shallower than that reported for the evolution of Lyman break galaxies (LBGs) at z > 4 (). Therefore, we conclude the LBGs likely represent a subset of highly star-forming galaxies that exhibit rapid size growth at z > 4.

    Original languageEnglish
    Article numberL11
    Pages (from-to)1-7
    Number of pages7
    JournalAstrophysical Journal Letters
    Volume834
    Issue number2
    DOIs
    Publication statusPublished - 10 Jan 2017

    Bibliographical note

    Copyright 2017 The American Astronomical Society. First published in Astrophysical Journal Letters, 834(2), L11. The original publication is available at https://doi.org/10.3847/2041-8213/834/2/L11, published by IOP Publishing. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.

    Keywords

    • galaxies: evolution
    • galaxies: high-redshift
    • galaxies: structure

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