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  • 1903.08171v1

    Rights statement: This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-4357/ab2f81.

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Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization

Research output: Contribution to journalJournal article

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  • J. Matthee
  • D. Sobral
  • L. A. Boogaard
  • H. Röttgering
  • L. Vallini
  • A. Ferrara
  • A. Paulino-Afonso
  • F. Boone
  • D. Schaerer
  • B. Mobasher
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Article number124
<mark>Journal publication date</mark>21/08/2019
<mark>Journal</mark>The Astrophysical Journal
Issue number2
Volume881
Number of pages20
Publication statusPublished
Original languageEnglish

Abstract

We present new deep ALMA and HST/WFC3 observations of MASOSA and VR7, two luminous Ly$\alpha$ emitters (LAEs) at $z=6.5$, for which the UV continuum level differ by a factor four. No IR dust continuum emission is detected in either, indicating little amounts of obscured star formation and/or high dust temperatures. MASOSA, with a UV luminosity M$_{1500}=-20.9$, compact size and very high Ly$\alpha$ EW$_{0}\approx145$ A, is undetected in [CII] to a limit of L$_{\rm [CII]}

Bibliographic note

This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-4357/ab2f81.