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    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

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Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization. / Matthee, J.; Sobral, D.; Boogaard, L. A. et al.
In: The Astrophysical Journal, Vol. 881, No. 2, 124, 21.08.2019.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Matthee, J, Sobral, D, Boogaard, LA, Röttgering, H, Vallini, L, Ferrara, A, Paulino-Afonso, A, Boone, F, Schaerer, D & Mobasher, B 2019, 'Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization', The Astrophysical Journal, vol. 881, no. 2, 124. https://doi.org/10.3847/1538-4357/ab2f81

APA

Matthee, J., Sobral, D., Boogaard, L. A., Röttgering, H., Vallini, L., Ferrara, A., Paulino-Afonso, A., Boone, F., Schaerer, D., & Mobasher, B. (2019). Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization. The Astrophysical Journal, 881(2), Article 124. https://doi.org/10.3847/1538-4357/ab2f81

Vancouver

Matthee J, Sobral D, Boogaard LA, Röttgering H, Vallini L, Ferrara A et al. Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization. The Astrophysical Journal. 2019 Aug 21;881(2):124. doi: 10.3847/1538-4357/ab2f81

Author

Matthee, J. ; Sobral, D. ; Boogaard, L. A. et al. / Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization. In: The Astrophysical Journal. 2019 ; Vol. 881, No. 2.

Bibtex

@article{93f69f30bd0a487589e6bdf04b874dfa,
title = "Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization",
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]}",
keywords = "astro-ph.GA",
author = "J. Matthee and D. Sobral and Boogaard, {L. A.} and H. R{\"o}ttgering and L. Vallini and A. Ferrara and A. Paulino-Afonso and F. Boone and D. Schaerer and B. Mobasher",
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.",
year = "2019",
month = aug,
day = "21",
doi = "10.3847/1538-4357/ab2f81",
language = "English",
volume = "881",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization

AU - Matthee, J.

AU - Sobral, D.

AU - Boogaard, L. A.

AU - Röttgering, H.

AU - Vallini, L.

AU - Ferrara, A.

AU - Paulino-Afonso, A.

AU - Boone, F.

AU - Schaerer, D.

AU - Mobasher, B.

N1 - 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.

PY - 2019/8/21

Y1 - 2019/8/21

N2 - 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]}

AB - 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]}

KW - astro-ph.GA

U2 - 10.3847/1538-4357/ab2f81

DO - 10.3847/1538-4357/ab2f81

M3 - Journal article

VL - 881

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 124

ER -