The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History
We present an original phenomenological model to describe the evolution of galaxy number counts, morphologies, and spectral energy distributions across a wide range of redshifts (0.2 < z < 15) and stellar masses [log(M M) ≤ 6]. Our model follows observed mass and luminosity functions of both s...
| Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2018 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/199458 |
| Acceso en línea: | http://hdl.handle.net/10261/199458 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxies: evolution Galaxies: high redshift Galaxies: photometry |
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The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic HistoryWilliams, Christina C.Curtis-Lake, E.Hainline, K. N.Chevallard, J.Robertson, B. E.Charlot, S.Endsley, R.Stark, Daniel P.Willmer, Christopher N. A.Alberts, S.Amorín, R.Arribas-Mocoroa, SantiagoBaum, S.Bunker, A.Carniani, S.Crandall, S.Egami, E.Eisenstein, Daniel J.Ferruit, P.Husemann, BerndMaseda, M. V.Maiolino, R.Rawle, Timothy D.Rieke, Marcia J.Smit, R.Tacchella, S.Willott, C. J.Galaxies: evolutionGalaxies: high redshiftGalaxies: photometryWe present an original phenomenological model to describe the evolution of galaxy number counts, morphologies, and spectral energy distributions across a wide range of redshifts (0.2 < z < 15) and stellar masses [log(M M) ≤ 6]. Our model follows observed mass and luminosity functions of both star-forming and quiescent galaxies, and reproduces the redshift evolution of colors, sizes, star formation, and chemical properties of the observed galaxy population. Unlike other existing approaches, our model includes a self-consistent treatment of stellar and photoionized gas emission and dust attenuation based on the BEAGLE tool. The mock galaxy catalogs generated with our new model can be used to simulate and optimize extragalactic surveys with future facilities such as the James Webb Space Telescope (JWST), and to enable critical assessments of analysis procedures, interpretation tools, and measurement systematics for both photometric and spectroscopic data. As a first application of this work, we make predictions for the upcoming JWST Advanced Deep Extragalactic Survey (JADES), a joint program of the JWST/NIRCam and NIRSpec Guaranteed Time Observations teams. We show that JADES will detect, with NIRCam imaging, 1000s of galaxies at z ≳6, and 10s at z ≳10 at m ≲ 30 (5δ) within the 236 arcmin2 of the survey. The JADES data will enable accurate constraints on the evolution of the UV luminosity function at z > 8, and resolve the current debate about the rate of evolution of galaxies at z≳8. Readyto- use mock catalogs and software to generate new realizations are publicly available as the JAdes extragalactic Ultradeep Artificial Realizations (JAGUAR) package.IOP PublishingConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2020202020182020info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/199458reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.3847/1538-4365/aabcbbSíinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1994582026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History |
| title |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History |
| spellingShingle |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History Williams, Christina C. Galaxies: evolution Galaxies: high redshift Galaxies: photometry |
| title_short |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History |
| title_full |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History |
| title_fullStr |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History |
| title_full_unstemmed |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History |
| title_sort |
The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History |
| dc.creator.none.fl_str_mv |
Williams, Christina C. Curtis-Lake, E. Hainline, K. N. Chevallard, J. Robertson, B. E. Charlot, S. Endsley, R. Stark, Daniel P. Willmer, Christopher N. A. Alberts, S. Amorín, R. Arribas-Mocoroa, Santiago Baum, S. Bunker, A. Carniani, S. Crandall, S. Egami, E. Eisenstein, Daniel J. Ferruit, P. Husemann, Bernd Maseda, M. V. Maiolino, R. Rawle, Timothy D. Rieke, Marcia J. Smit, R. Tacchella, S. Willott, C. J. |
| author |
Williams, Christina C. |
| author_facet |
Williams, Christina C. Curtis-Lake, E. Hainline, K. N. Chevallard, J. Robertson, B. E. Charlot, S. Endsley, R. Stark, Daniel P. Willmer, Christopher N. A. Alberts, S. Amorín, R. Arribas-Mocoroa, Santiago Baum, S. Bunker, A. Carniani, S. Crandall, S. Egami, E. Eisenstein, Daniel J. Ferruit, P. Husemann, Bernd Maseda, M. V. Maiolino, R. Rawle, Timothy D. Rieke, Marcia J. Smit, R. Tacchella, S. Willott, C. J. |
| author_role |
author |
| author2 |
Curtis-Lake, E. Hainline, K. N. Chevallard, J. Robertson, B. E. Charlot, S. Endsley, R. Stark, Daniel P. Willmer, Christopher N. A. Alberts, S. Amorín, R. Arribas-Mocoroa, Santiago Baum, S. Bunker, A. Carniani, S. Crandall, S. Egami, E. Eisenstein, Daniel J. Ferruit, P. Husemann, Bernd Maseda, M. V. Maiolino, R. Rawle, Timothy D. Rieke, Marcia J. Smit, R. Tacchella, S. Willott, C. J. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Galaxies: evolution Galaxies: high redshift Galaxies: photometry |
| topic |
Galaxies: evolution Galaxies: high redshift Galaxies: photometry |
| description |
We present an original phenomenological model to describe the evolution of galaxy number counts, morphologies, and spectral energy distributions across a wide range of redshifts (0.2 < z < 15) and stellar masses [log(M M) ≤ 6]. Our model follows observed mass and luminosity functions of both star-forming and quiescent galaxies, and reproduces the redshift evolution of colors, sizes, star formation, and chemical properties of the observed galaxy population. Unlike other existing approaches, our model includes a self-consistent treatment of stellar and photoionized gas emission and dust attenuation based on the BEAGLE tool. The mock galaxy catalogs generated with our new model can be used to simulate and optimize extragalactic surveys with future facilities such as the James Webb Space Telescope (JWST), and to enable critical assessments of analysis procedures, interpretation tools, and measurement systematics for both photometric and spectroscopic data. As a first application of this work, we make predictions for the upcoming JWST Advanced Deep Extragalactic Survey (JADES), a joint program of the JWST/NIRCam and NIRSpec Guaranteed Time Observations teams. We show that JADES will detect, with NIRCam imaging, 1000s of galaxies at z ≳6, and 10s at z ≳10 at m ≲ 30 (5δ) within the 236 arcmin2 of the survey. The JADES data will enable accurate constraints on the evolution of the UV luminosity function at z > 8, and resolve the current debate about the rate of evolution of galaxies at z≳8. Readyto- use mock catalogs and software to generate new realizations are publicly available as the JAdes extragalactic Ultradeep Artificial Realizations (JAGUAR) package. |
| publishDate |
2018 |
| dc.date.none.fl_str_mv |
2018 2020 2020 2020 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/199458 |
| url |
http://hdl.handle.net/10261/199458 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
http://dx.doi.org/10.3847/1538-4365/aabcbb Sí |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
| eu_rights_str_mv |
openAccess |
| dc.publisher.none.fl_str_mv |
IOP Publishing |
| publisher.none.fl_str_mv |
IOP Publishing |
| dc.source.none.fl_str_mv |
reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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1869405574450380800 |
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15,228081 |