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Conference object . 2017
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The Luminosity-Dependent Clustering Of Hα Emitters From Z~0.8 To Z~2.2 With Hizels

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 13 Jun 2017Publisher:Zenodo
Authors: Cochrane, R. K.;

doi: 10.5281/zenodo.807604 , 10.5281/zenodo.807603

The Luminosity-Dependent Clustering Of Hα Emitters From Z~0.8 To Z~2.2 With Hizels

Abstract

Poster presented at the conference Galaxy evoltion Across Time, 12-16 June, Paris, France We study the clustering of star-forming galaxies, using halo models to derive dark matter halo masses. Typical galaxies in our samples are star-forming centrals, residing in host halos of mass 10^12 M_solar. We find strong trends between galaxy Hα luminosity and dark matter halo mass at all redshifts. See also https://arxiv.org/abs/1704.05472

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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).
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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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