MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ∼ −15-Reference-Cited by-同舟云学术

MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ∼ −15

Published:2018-09-14 Issue:1 Volume:865 Page:L1
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Maseda Michael V.^ORCID,Bacon Roland,Franx Marijn^ORCID,Brinchmann Jarle^ORCID,Schaye Joop^ORCID,Boogaard Leindert A.^ORCID,Bouché Nicolas^ORCID,Bouwens Rychard J.^ORCID,Cantalupo Sebastiano,Contini Thierry^ORCID,Hashimoto Takuya^ORCID,Inami Hanae,Marino Raffaella A.^ORCID,Muzahid Sowgat^ORCID,Nanayakkara Themiya^ORCID,Richard Johan^ORCID,Schmidt Kasper B.^ORCID,Verhamme Anne^ORCID,Wisotzki Lutz

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/aade4b/pdf

Reference38 articles.

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5. LOWER-LUMINOSITY GALAXIES COULD REIONIZE THE UNIVERSE: VERY STEEP FAINT-END SLOPES TO THE UV LUMINOSITY FUNCTIONS AT z ⩾ 5-8 FROM THE HUDF09 WFC3/IR OBSERVATIONS

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