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
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Author / Creator
Valentino, F , Daddi, E , Silverman, J D , Puglisi, A , Kashino, D , Renzini, A , Cimatti, A , Pozzetti, L , Rodighiero, G , Pannella, M , Gobat, R and Zamorani, G
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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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...
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Full title
Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys
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Record Identifier
TN_cdi_proquest_journals_2076569851
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2076569851
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1709.01936