z≳ 7 galaxies with red SPITZER/IRAC [3.6]--[4.5] colors in the full CANDELS data set: The brightest-known galaxies at z~ 7--9 and a probable spectroscopic confirmation at z= 7.48: The brightest-known galaxies at z ∼ 7-9 and a probable spectroscopic confirmation at z = 7.48

GW Roberts-Borsani, RJ Bouwens, PA Oesch, I Labbe, R Smit, GD Illingworth, P van Dokkum, B Holden, V Gonzalez, M Stefanon, Adi Zitrin

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122 Scopus citations

Abstract

We identify four unusually bright (H160,AB < 25.5) galaxies from Hubble Space Telescope (HST) and Spitzer CANDELS data with probable redshifts z ∼ 7–9. These identifications include the brightest-known galaxies to date at z  7.5. As Y-band observations are not available over the full CANDELS program to perform a standard Lyman-break selection of z > 7 galaxies, we employ an alternate strategy using deep Spitzer/IRAC data. We identify z ∼ 7.1–9.1 galaxies by selecting z  6 galaxies from the HST CANDELS data that show quite red IRAC
[3.6]−[4.5] colors, indicating strong [O III]+Hβ lines in the 4.5 μm band. This selection strategy was validated using a modest sample for which we have deep Y-band coverage, and subsequently used to select the brightest z … 7 sources. Applying the IRAC criteria to all HST-selected optical dropout galaxies over the full ∼900 arcmin2 of the CANDELS survey revealed four unusually bright z ∼ 7.1, 7.6, 7.9, and 8.6 candidates. The median [3.6]−[4.5] color of our selected z ∼ 7.1–9.1 sample is consistent with rest-frame [O III]+Hβ EWs of ∼1500 Å in the [4.5] band. Keck/MOSFIRE spectroscopy has been independently reported for two of our selected sources, showing Lyα at redshifts of 7.7302 ± 0.0006 and -
+ 8.683 0.004 0.001, respectively. We present similar Keck/MOSFIRE
spectroscopy for a third selected galaxy with a probable 4.7σ Lyα line at zspec = 7.4770 ± 0.0008. All three have H160-band magnitudes of ∼25 mag and are ∼0.5 mag more luminous (M1600 ∼ −22.0) than any previously discovered z ∼ 8 galaxy, with important implications for the UV luminosity function (LF). Our three brightest and highest redshift z > 7 galaxies all lie within the CANDELS-EGS field, providing a dramatic illustration of the potential impact of field-to-field variance.
Original languageEnglish GB
Article number143
Pages (from-to)143
Number of pages1
JournalThe Astrophysical Journal
Volume823
Issue number2
DOIs
StatePublished - 2016

Keywords

  • galaxies
  • evolution
  • galaxies: high-redshift

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