The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15
The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Bingjie Wang [verfasserIn] Joel Leja [verfasserIn] Ivo Labbé [verfasserIn] Rachel Bezanson [verfasserIn] Katherine E. Whitaker [verfasserIn] Gabriel Brammer [verfasserIn] Lukas J. Furtak [verfasserIn] John R. Weaver [verfasserIn] Sedona H. Price [verfasserIn] Adi Zitrin [verfasserIn] Hakim Atek [verfasserIn] Dan Coe [verfasserIn] Sam E. Cutler [verfasserIn] Pratika Dayal [verfasserIn] Pieter van Dokkum [verfasserIn] Robert Feldmann [verfasserIn] Danilo Marchesini [verfasserIn] Marijn Franx [verfasserIn] Natascha Förster Schreiber [verfasserIn] Seiji Fujimoto [verfasserIn] Marla Geha [verfasserIn] Karl Glazebrook [verfasserIn] Anna de Graaff [verfasserIn] Jenny E. Greene [verfasserIn] Stéphanie Juneau [verfasserIn] Susan Kassin [verfasserIn] Mariska Kriek [verfasserIn] Gourav Khullar [verfasserIn] Michael Maseda [verfasserIn] Lamiya A. Mowla [verfasserIn] Adam Muzzin [verfasserIn] Themiya Nanayakkara [verfasserIn] Erica J. Nelson [verfasserIn] Pascal A. Oesch [verfasserIn] Camilla Pacifici [verfasserIn] Richard Pan [verfasserIn] Casey Papovich [verfasserIn] David J. Setton [verfasserIn] Alice E. Shapley [verfasserIn] Renske Smit [verfasserIn] Mauro Stefanon [verfasserIn] Katherine A. Suess [verfasserIn] Edward N. Taylor [verfasserIn] Christina C. Williams [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
In: The Astrophysical Journal Supplement Series - IOP Publishing, 2022, 270(2023), 1, p 12 |
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| Übergeordnetes Werk: |
volume:270 ; year:2023 ; number:1, p 12 |
| Links: |
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| DOI / URN: |
10.3847/1538-4365/ad0846 |
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| Katalog-ID: |
DOAJ09803975X |
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| 245 | 1 | 4 | |a The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 |
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| 520 | |a The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. | ||
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| 700 | 0 | |a Christina C. Williams |e verfasserin |4 aut | |
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10.3847/1538-4365/ad0846 doi (DE-627)DOAJ09803975X (DE-599)DOAJa36ada68a6c04784822f143af2de06e4 DE-627 ger DE-627 rakwb eng QB460-466 Bingjie Wang verfasserin aut The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. Abell clusters Catalogs Galaxy evolution James Webb Space Telescope Hubble Space Telescope Spectral energy distribution Astrophysics Joel Leja verfasserin aut Ivo Labbé verfasserin aut Rachel Bezanson verfasserin aut Katherine E. Whitaker verfasserin aut Gabriel Brammer verfasserin aut Lukas J. Furtak verfasserin aut John R. Weaver verfasserin aut Sedona H. Price verfasserin aut Adi Zitrin verfasserin aut Hakim Atek verfasserin aut Dan Coe verfasserin aut Sam E. Cutler verfasserin aut Pratika Dayal verfasserin aut Pieter van Dokkum verfasserin aut Robert Feldmann verfasserin aut Danilo Marchesini verfasserin aut Marijn Franx verfasserin aut Natascha Förster Schreiber verfasserin aut Seiji Fujimoto verfasserin aut Marla Geha verfasserin aut Karl Glazebrook verfasserin aut Anna de Graaff verfasserin aut Jenny E. Greene verfasserin aut Stéphanie Juneau verfasserin aut Susan Kassin verfasserin aut Mariska Kriek verfasserin aut Gourav Khullar verfasserin aut Michael Maseda verfasserin aut Lamiya A. Mowla verfasserin aut Adam Muzzin verfasserin aut Themiya Nanayakkara verfasserin aut Erica J. Nelson verfasserin aut Pascal A. Oesch verfasserin aut Camilla Pacifici verfasserin aut Richard Pan verfasserin aut Casey Papovich verfasserin aut David J. Setton verfasserin aut Alice E. Shapley verfasserin aut Renske Smit verfasserin aut Mauro Stefanon verfasserin aut Katherine A. Suess verfasserin aut Edward N. Taylor verfasserin aut Christina C. Williams verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 270(2023), 1, p 12 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:270 year:2023 number:1, p 12 https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/article/a36ada68a6c04784822f143af2de06e4 kostenfrei https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/toc/0067-0049 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 270 2023 1, p 12 |
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10.3847/1538-4365/ad0846 doi (DE-627)DOAJ09803975X (DE-599)DOAJa36ada68a6c04784822f143af2de06e4 DE-627 ger DE-627 rakwb eng QB460-466 Bingjie Wang verfasserin aut The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. Abell clusters Catalogs Galaxy evolution James Webb Space Telescope Hubble Space Telescope Spectral energy distribution Astrophysics Joel Leja verfasserin aut Ivo Labbé verfasserin aut Rachel Bezanson verfasserin aut Katherine E. Whitaker verfasserin aut Gabriel Brammer verfasserin aut Lukas J. Furtak verfasserin aut John R. Weaver verfasserin aut Sedona H. Price verfasserin aut Adi Zitrin verfasserin aut Hakim Atek verfasserin aut Dan Coe verfasserin aut Sam E. Cutler verfasserin aut Pratika Dayal verfasserin aut Pieter van Dokkum verfasserin aut Robert Feldmann verfasserin aut Danilo Marchesini verfasserin aut Marijn Franx verfasserin aut Natascha Förster Schreiber verfasserin aut Seiji Fujimoto verfasserin aut Marla Geha verfasserin aut Karl Glazebrook verfasserin aut Anna de Graaff verfasserin aut Jenny E. Greene verfasserin aut Stéphanie Juneau verfasserin aut Susan Kassin verfasserin aut Mariska Kriek verfasserin aut Gourav Khullar verfasserin aut Michael Maseda verfasserin aut Lamiya A. Mowla verfasserin aut Adam Muzzin verfasserin aut Themiya Nanayakkara verfasserin aut Erica J. Nelson verfasserin aut Pascal A. Oesch verfasserin aut Camilla Pacifici verfasserin aut Richard Pan verfasserin aut Casey Papovich verfasserin aut David J. Setton verfasserin aut Alice E. Shapley verfasserin aut Renske Smit verfasserin aut Mauro Stefanon verfasserin aut Katherine A. Suess verfasserin aut Edward N. Taylor verfasserin aut Christina C. Williams verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 270(2023), 1, p 12 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:270 year:2023 number:1, p 12 https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/article/a36ada68a6c04784822f143af2de06e4 kostenfrei https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/toc/0067-0049 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 270 2023 1, p 12 |
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10.3847/1538-4365/ad0846 doi (DE-627)DOAJ09803975X (DE-599)DOAJa36ada68a6c04784822f143af2de06e4 DE-627 ger DE-627 rakwb eng QB460-466 Bingjie Wang verfasserin aut The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. Abell clusters Catalogs Galaxy evolution James Webb Space Telescope Hubble Space Telescope Spectral energy distribution Astrophysics Joel Leja verfasserin aut Ivo Labbé verfasserin aut Rachel Bezanson verfasserin aut Katherine E. Whitaker verfasserin aut Gabriel Brammer verfasserin aut Lukas J. Furtak verfasserin aut John R. Weaver verfasserin aut Sedona H. Price verfasserin aut Adi Zitrin verfasserin aut Hakim Atek verfasserin aut Dan Coe verfasserin aut Sam E. Cutler verfasserin aut Pratika Dayal verfasserin aut Pieter van Dokkum verfasserin aut Robert Feldmann verfasserin aut Danilo Marchesini verfasserin aut Marijn Franx verfasserin aut Natascha Förster Schreiber verfasserin aut Seiji Fujimoto verfasserin aut Marla Geha verfasserin aut Karl Glazebrook verfasserin aut Anna de Graaff verfasserin aut Jenny E. Greene verfasserin aut Stéphanie Juneau verfasserin aut Susan Kassin verfasserin aut Mariska Kriek verfasserin aut Gourav Khullar verfasserin aut Michael Maseda verfasserin aut Lamiya A. Mowla verfasserin aut Adam Muzzin verfasserin aut Themiya Nanayakkara verfasserin aut Erica J. Nelson verfasserin aut Pascal A. Oesch verfasserin aut Camilla Pacifici verfasserin aut Richard Pan verfasserin aut Casey Papovich verfasserin aut David J. Setton verfasserin aut Alice E. Shapley verfasserin aut Renske Smit verfasserin aut Mauro Stefanon verfasserin aut Katherine A. Suess verfasserin aut Edward N. Taylor verfasserin aut Christina C. Williams verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 270(2023), 1, p 12 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:270 year:2023 number:1, p 12 https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/article/a36ada68a6c04784822f143af2de06e4 kostenfrei https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/toc/0067-0049 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 270 2023 1, p 12 |
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10.3847/1538-4365/ad0846 doi (DE-627)DOAJ09803975X (DE-599)DOAJa36ada68a6c04784822f143af2de06e4 DE-627 ger DE-627 rakwb eng QB460-466 Bingjie Wang verfasserin aut The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. Abell clusters Catalogs Galaxy evolution James Webb Space Telescope Hubble Space Telescope Spectral energy distribution Astrophysics Joel Leja verfasserin aut Ivo Labbé verfasserin aut Rachel Bezanson verfasserin aut Katherine E. Whitaker verfasserin aut Gabriel Brammer verfasserin aut Lukas J. Furtak verfasserin aut John R. Weaver verfasserin aut Sedona H. Price verfasserin aut Adi Zitrin verfasserin aut Hakim Atek verfasserin aut Dan Coe verfasserin aut Sam E. Cutler verfasserin aut Pratika Dayal verfasserin aut Pieter van Dokkum verfasserin aut Robert Feldmann verfasserin aut Danilo Marchesini verfasserin aut Marijn Franx verfasserin aut Natascha Förster Schreiber verfasserin aut Seiji Fujimoto verfasserin aut Marla Geha verfasserin aut Karl Glazebrook verfasserin aut Anna de Graaff verfasserin aut Jenny E. Greene verfasserin aut Stéphanie Juneau verfasserin aut Susan Kassin verfasserin aut Mariska Kriek verfasserin aut Gourav Khullar verfasserin aut Michael Maseda verfasserin aut Lamiya A. Mowla verfasserin aut Adam Muzzin verfasserin aut Themiya Nanayakkara verfasserin aut Erica J. Nelson verfasserin aut Pascal A. Oesch verfasserin aut Camilla Pacifici verfasserin aut Richard Pan verfasserin aut Casey Papovich verfasserin aut David J. Setton verfasserin aut Alice E. Shapley verfasserin aut Renske Smit verfasserin aut Mauro Stefanon verfasserin aut Katherine A. Suess verfasserin aut Edward N. Taylor verfasserin aut Christina C. Williams verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 270(2023), 1, p 12 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:270 year:2023 number:1, p 12 https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/article/a36ada68a6c04784822f143af2de06e4 kostenfrei https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/toc/0067-0049 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 270 2023 1, p 12 |
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10.3847/1538-4365/ad0846 doi (DE-627)DOAJ09803975X (DE-599)DOAJa36ada68a6c04784822f143af2de06e4 DE-627 ger DE-627 rakwb eng QB460-466 Bingjie Wang verfasserin aut The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. Abell clusters Catalogs Galaxy evolution James Webb Space Telescope Hubble Space Telescope Spectral energy distribution Astrophysics Joel Leja verfasserin aut Ivo Labbé verfasserin aut Rachel Bezanson verfasserin aut Katherine E. Whitaker verfasserin aut Gabriel Brammer verfasserin aut Lukas J. Furtak verfasserin aut John R. Weaver verfasserin aut Sedona H. Price verfasserin aut Adi Zitrin verfasserin aut Hakim Atek verfasserin aut Dan Coe verfasserin aut Sam E. Cutler verfasserin aut Pratika Dayal verfasserin aut Pieter van Dokkum verfasserin aut Robert Feldmann verfasserin aut Danilo Marchesini verfasserin aut Marijn Franx verfasserin aut Natascha Förster Schreiber verfasserin aut Seiji Fujimoto verfasserin aut Marla Geha verfasserin aut Karl Glazebrook verfasserin aut Anna de Graaff verfasserin aut Jenny E. Greene verfasserin aut Stéphanie Juneau verfasserin aut Susan Kassin verfasserin aut Mariska Kriek verfasserin aut Gourav Khullar verfasserin aut Michael Maseda verfasserin aut Lamiya A. Mowla verfasserin aut Adam Muzzin verfasserin aut Themiya Nanayakkara verfasserin aut Erica J. Nelson verfasserin aut Pascal A. Oesch verfasserin aut Camilla Pacifici verfasserin aut Richard Pan verfasserin aut Casey Papovich verfasserin aut David J. Setton verfasserin aut Alice E. Shapley verfasserin aut Renske Smit verfasserin aut Mauro Stefanon verfasserin aut Katherine A. Suess verfasserin aut Edward N. Taylor verfasserin aut Christina C. Williams verfasserin aut In The Astrophysical Journal Supplement Series IOP Publishing, 2022 270(2023), 1, p 12 (DE-627)312200196 (DE-600)2006860-8 15384365 nnns volume:270 year:2023 number:1, p 12 https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/article/a36ada68a6c04784822f143af2de06e4 kostenfrei https://doi.org/10.3847/1538-4365/ad0846 kostenfrei https://doaj.org/toc/0067-0049 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 270 2023 1, p 12 |
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Bingjie Wang @@aut@@ Joel Leja @@aut@@ Ivo Labbé @@aut@@ Rachel Bezanson @@aut@@ Katherine E. Whitaker @@aut@@ Gabriel Brammer @@aut@@ Lukas J. Furtak @@aut@@ John R. Weaver @@aut@@ Sedona H. Price @@aut@@ Adi Zitrin @@aut@@ Hakim Atek @@aut@@ Dan Coe @@aut@@ Sam E. Cutler @@aut@@ Pratika Dayal @@aut@@ Pieter van Dokkum @@aut@@ Robert Feldmann @@aut@@ Danilo Marchesini @@aut@@ Marijn Franx @@aut@@ Natascha Förster Schreiber @@aut@@ Seiji Fujimoto @@aut@@ Marla Geha @@aut@@ Karl Glazebrook @@aut@@ Anna de Graaff @@aut@@ Jenny E. Greene @@aut@@ Stéphanie Juneau @@aut@@ Susan Kassin @@aut@@ Mariska Kriek @@aut@@ Gourav Khullar @@aut@@ Michael Maseda @@aut@@ Lamiya A. Mowla @@aut@@ Adam Muzzin @@aut@@ Themiya Nanayakkara @@aut@@ Erica J. Nelson @@aut@@ Pascal A. Oesch @@aut@@ Camilla Pacifici @@aut@@ Richard Pan @@aut@@ Casey Papovich @@aut@@ David J. Setton @@aut@@ Alice E. Shapley @@aut@@ Renske Smit @@aut@@ Mauro Stefanon @@aut@@ Katherine A. Suess @@aut@@ Edward N. Taylor @@aut@@ Christina C. Williams @@aut@@ |
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uncover survey: a first-look hst+jwst catalog of galaxy redshifts and stellar population properties spanning 0.2 ≲ z ≲ 15 |
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The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 |
| abstract |
The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. |
| abstractGer |
The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. |
| abstract_unstemmed |
The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster A2744 to create the deepest view of our Universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of more than 50,000 robustly detected sources out to z ∼ 15. We show the redshift evolution of stellar ages, star formation rates, and rest-frame colors across the full range of 0.2 ≲ z ≲ 15. The galaxy properties are inferred using the Prospector Bayesian inference framework using informative Prospector - β priors on the masses and star formation histories to produce joint redshift and stellar populations posteriors. Additionally, lensing magnification is performed on the fly to ensure consistency with the scale-dependent priors. We show that this approach produces excellent photometric redshifts with σ _NMAD ∼ 0.03, of a similar quality to the established photometric redshift code EAzY . In line with the open-source scientific objective of this Treasury survey, we publicly release the stellar population catalog with this paper, derived from our photometric catalog adapting aperture sizes based on source profiles. This release (the catalog and all related documentation are accessible via the UNCOVER survey web page: https://jwst-uncover.github.io/DR2.html#SPSCatalogs with a copy deposited to Zenodo at doi: https://doi.org/10.5281/zenodo.8401181 ) includes posterior moments, maximum likelihood spectra, star formation histories, and full posterior distributions, offering a rich data set to explore the processes governing galaxy formation and evolution over a parameter space now accessible by JWST. |
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1, p 12 |
| title_short |
The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning 0.2 ≲ z ≲ 15 |
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https://doi.org/10.3847/1538-4365/ad0846 https://doaj.org/article/a36ada68a6c04784822f143af2de06e4 https://doaj.org/toc/0067-0049 |
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Joel Leja Ivo Labbé Rachel Bezanson Katherine E. Whitaker Gabriel Brammer Lukas J. Furtak John R. Weaver Sedona H. Price Adi Zitrin Hakim Atek Dan Coe Sam E. Cutler Pratika Dayal Pieter van Dokkum Robert Feldmann Danilo Marchesini Marijn Franx Natascha Förster Schreiber Seiji Fujimoto Marla Geha Karl Glazebrook Anna de Graaff Jenny E. Greene Stéphanie Juneau Susan Kassin Mariska Kriek Gourav Khullar Michael Maseda Lamiya A. Mowla Adam Muzzin Themiya Nanayakkara Erica J. Nelson Pascal A. Oesch Camilla Pacifici Richard Pan Casey Papovich David J. Setton Alice E. Shapley Renske Smit Mauro Stefanon Katherine A. Suess Edward N. Taylor Christina C. Williams |
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Joel Leja Ivo Labbé Rachel Bezanson Katherine E. Whitaker Gabriel Brammer Lukas J. Furtak John R. Weaver Sedona H. Price Adi Zitrin Hakim Atek Dan Coe Sam E. Cutler Pratika Dayal Pieter van Dokkum Robert Feldmann Danilo Marchesini Marijn Franx Natascha Förster Schreiber Seiji Fujimoto Marla Geha Karl Glazebrook Anna de Graaff Jenny E. Greene Stéphanie Juneau Susan Kassin Mariska Kriek Gourav Khullar Michael Maseda Lamiya A. Mowla Adam Muzzin Themiya Nanayakkara Erica J. Nelson Pascal A. Oesch Camilla Pacifici Richard Pan Casey Papovich David J. Setton Alice E. Shapley Renske Smit Mauro Stefanon Katherine A. Suess Edward N. Taylor Christina C. Williams |
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