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Monthly Notices of the Royal Astronomical Society
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Monthly Notices of the Royal Astronomical Society
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https://dx.doi.org/10.48550/ar...
Article . 2017
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The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5

descriptionPublicationkeyboard_double_arrow_right Article 30 Oct 2017Embargo end date: 01 Jan 2017 United Kingdom English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 474, pages 4,024-4,038 (issn: 0035-8711, eissn: 1365-2966, Copyright policy )
Authors: V Gonzalez-Perez; J Comparat; P Norberg; C M Baugh; S Contreras; C Lacey; N McCullagh; +3 Authors

doi: 10.1093/mnras/stx2807 , 10.48550/arxiv.1708.07628

The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5

Abstract

Emission line galaxies (ELGs) are used in several ongoing and upcoming surveys (SDSS-IV/eBOSS, DESI) as tracers of the dark matter distribution. Using a new galaxy formation model, we explore the characteristics of [OII] emitters, which dominate optical ELG selections at $z\simeq 1$. Model [OII] emitters at $0.5

17 pages, 16 figures, MNRAS

Country
United Kingdom
Related Organizations
Keywords

theory [cosmology], Cosmology and Nongalactic Astrophysics (astro-ph.CO), formation [galaxies], astro-ph.GA, RCUK, ST/K00087X/1, FOS: Physical sciences, numerical [methods], ST/K003267/1, ST/K00042X/1, ST/H008519/1, analytical [methods], Astrophysics of Galaxies (astro-ph.GA), astro-ph.CO, ST/L00075X/1, STFC, evolution [galaxies]

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    influence
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    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
69
Top 10%
Top 10%
Top 1%
Green
gold