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Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys

Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2076569851

Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys

About this item

Full title

Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2017-09

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

We estimate the number counts of line emitters at high redshift and their evolution with cosmic time based on a combination of photometry and spectroscopy. We predict the H\(\alpha\), H\(\beta\), [OII], and [OIII] line fluxes for more than \(35,000\) galaxies down to stellar masses of \(\sim10^9\) \(M_{\odot}\) in the COSMOS and GOODS-S fields, app...

Alternative Titles

Full title

Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2076569851

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2076569851

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1709.01936

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