Tracing dark matter overdensities with dusty star-forming galaxies
It has been suggested that associations of high-redshift dusty star-forming galaxies (DSFGs) may serve as beacons of protoclusters because DSFGs are high-mass galaxies undergoing rapid assembly. We investigate this possibility using the Bolshoi cosmological N-body simulation and a model for populati...
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ftdatacite:10.5281/zenodo.3518811 2023-05-15T18:22:15+02:00 Tracing dark matter overdensities with dusty star-forming galaxies Hayward, Christopher C. 2019 https://dx.doi.org/10.5281/zenodo.3518811 https://zenodo.org/record/3518811 unknown Zenodo https://zenodo.org/communities/firstgalaxiesfirststructures https://dx.doi.org/10.5281/zenodo.3518810 https://zenodo.org/communities/firstgalaxiesfirststructures Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess CC-BY DSFGs protoclusters SMGs Text Presentation article-journal ScholarlyArticle 2019 ftdatacite https://doi.org/10.5281/zenodo.3518811 https://doi.org/10.5281/zenodo.3518810 2021-11-05T12:55:41Z It has been suggested that associations of high-redshift dusty star-forming galaxies (DSFGs) may serve as beacons of protoclusters because DSFGs are high-mass galaxies undergoing rapid assembly. We investigate this possibility using the Bolshoi cosmological N-body simulation and a model for populating the simulation with DSFGs. We find that DSFGs are incomplete tracers of protoclusters because of stochastic sampling effects, and at redshift <~ 2.5, because of ‘downsizing’, the highest dark matter overdensities are not well traced by DSFG associations. However, at high redshift, bright submm sources provide effective means for finding some of the most extreme dark matter overdensities in the Universe; I will discuss two such examples discovered with the South Pole Telescope. Conference Object South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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unknown |
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DSFGs protoclusters SMGs |
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DSFGs protoclusters SMGs Hayward, Christopher C. Tracing dark matter overdensities with dusty star-forming galaxies |
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DSFGs protoclusters SMGs |
description |
It has been suggested that associations of high-redshift dusty star-forming galaxies (DSFGs) may serve as beacons of protoclusters because DSFGs are high-mass galaxies undergoing rapid assembly. We investigate this possibility using the Bolshoi cosmological N-body simulation and a model for populating the simulation with DSFGs. We find that DSFGs are incomplete tracers of protoclusters because of stochastic sampling effects, and at redshift <~ 2.5, because of ‘downsizing’, the highest dark matter overdensities are not well traced by DSFG associations. However, at high redshift, bright submm sources provide effective means for finding some of the most extreme dark matter overdensities in the Universe; I will discuss two such examples discovered with the South Pole Telescope. |
format |
Conference Object |
author |
Hayward, Christopher C. |
author_facet |
Hayward, Christopher C. |
author_sort |
Hayward, Christopher C. |
title |
Tracing dark matter overdensities with dusty star-forming galaxies |
title_short |
Tracing dark matter overdensities with dusty star-forming galaxies |
title_full |
Tracing dark matter overdensities with dusty star-forming galaxies |
title_fullStr |
Tracing dark matter overdensities with dusty star-forming galaxies |
title_full_unstemmed |
Tracing dark matter overdensities with dusty star-forming galaxies |
title_sort |
tracing dark matter overdensities with dusty star-forming galaxies |
publisher |
Zenodo |
publishDate |
2019 |
url |
https://dx.doi.org/10.5281/zenodo.3518811 https://zenodo.org/record/3518811 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://zenodo.org/communities/firstgalaxiesfirststructures https://dx.doi.org/10.5281/zenodo.3518810 https://zenodo.org/communities/firstgalaxiesfirststructures |
op_rights |
Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.5281/zenodo.3518811 https://doi.org/10.5281/zenodo.3518810 |
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1766201645722501120 |