Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?

We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using...
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Autor*in:	Abdurro’uf [verfasserIn] Dan Coe [verfasserIn] Intae Jung [verfasserIn] Henry C. Ferguson [verfasserIn] Gabriel Brammer [verfasserIn] Kartheik G. Iyer [verfasserIn] Larry D. Bradley [verfasserIn] Pratika Dayal [verfasserIn] Rogier A. Windhorst [verfasserIn] Adi Zitrin [verfasserIn] Ashish Kumar Meena [verfasserIn] Masamune Oguri [verfasserIn] Jose M. Diego [verfasserIn] Vasily Kokorev [verfasserIn] Paola Dimauro [verfasserIn] Angela Adamo [verfasserIn] Christopher J. Conselice [verfasserIn] Brian Welch [verfasserIn] Eros Vanzella [verfasserIn] Tiger Yu-Yang Hsiao [verfasserIn] Xinfeng Xu [verfasserIn] Namrata Roy [verfasserIn] Celia R. Mulcahey [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 945(2023), 2, p 117
Übergeordnetes Werk:	volume:945 ; year:2023 ; number:2, p 117

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/acba06

Katalog-ID:	DOAJ089152085

Internformat


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245	1	0	\|a Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?
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allfields	10.3847/1538-4357/acba06 doi (DE-627)DOAJ089152085 (DE-599)DOAJ68a54c123198430287c00f66c141e47a DE-627 ger DE-627 rakwb eng QB460-466 Abdurro’uf verfasserin aut Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time? 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures. Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching Astrophysics Dan Coe verfasserin aut Intae Jung verfasserin aut Henry C. Ferguson verfasserin aut Gabriel Brammer verfasserin aut Kartheik G. Iyer verfasserin aut Larry D. Bradley verfasserin aut Pratika Dayal verfasserin aut Rogier A. Windhorst verfasserin aut Adi Zitrin verfasserin aut Ashish Kumar Meena verfasserin aut Masamune Oguri verfasserin aut Jose M. Diego verfasserin aut Vasily Kokorev verfasserin aut Paola Dimauro verfasserin aut Angela Adamo verfasserin aut Christopher J. Conselice verfasserin aut Brian Welch verfasserin aut Eros Vanzella verfasserin aut Tiger Yu-Yang Hsiao verfasserin aut Xinfeng Xu verfasserin aut Namrata Roy verfasserin aut Celia R. Mulcahey verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 945(2023), 2, p 117 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:945 year:2023 number:2, p 117 https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/article/68a54c123198430287c00f66c141e47a kostenfrei https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/toc/1538-4357 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_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 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 945 2023 2, p 117
spelling	10.3847/1538-4357/acba06 doi (DE-627)DOAJ089152085 (DE-599)DOAJ68a54c123198430287c00f66c141e47a DE-627 ger DE-627 rakwb eng QB460-466 Abdurro’uf verfasserin aut Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time? 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures. Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching Astrophysics Dan Coe verfasserin aut Intae Jung verfasserin aut Henry C. Ferguson verfasserin aut Gabriel Brammer verfasserin aut Kartheik G. Iyer verfasserin aut Larry D. Bradley verfasserin aut Pratika Dayal verfasserin aut Rogier A. Windhorst verfasserin aut Adi Zitrin verfasserin aut Ashish Kumar Meena verfasserin aut Masamune Oguri verfasserin aut Jose M. Diego verfasserin aut Vasily Kokorev verfasserin aut Paola Dimauro verfasserin aut Angela Adamo verfasserin aut Christopher J. Conselice verfasserin aut Brian Welch verfasserin aut Eros Vanzella verfasserin aut Tiger Yu-Yang Hsiao verfasserin aut Xinfeng Xu verfasserin aut Namrata Roy verfasserin aut Celia R. Mulcahey verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 945(2023), 2, p 117 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:945 year:2023 number:2, p 117 https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/article/68a54c123198430287c00f66c141e47a kostenfrei https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/toc/1538-4357 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_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 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 945 2023 2, p 117
allfields_unstemmed	10.3847/1538-4357/acba06 doi (DE-627)DOAJ089152085 (DE-599)DOAJ68a54c123198430287c00f66c141e47a DE-627 ger DE-627 rakwb eng QB460-466 Abdurro’uf verfasserin aut Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time? 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures. Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching Astrophysics Dan Coe verfasserin aut Intae Jung verfasserin aut Henry C. Ferguson verfasserin aut Gabriel Brammer verfasserin aut Kartheik G. Iyer verfasserin aut Larry D. Bradley verfasserin aut Pratika Dayal verfasserin aut Rogier A. Windhorst verfasserin aut Adi Zitrin verfasserin aut Ashish Kumar Meena verfasserin aut Masamune Oguri verfasserin aut Jose M. Diego verfasserin aut Vasily Kokorev verfasserin aut Paola Dimauro verfasserin aut Angela Adamo verfasserin aut Christopher J. Conselice verfasserin aut Brian Welch verfasserin aut Eros Vanzella verfasserin aut Tiger Yu-Yang Hsiao verfasserin aut Xinfeng Xu verfasserin aut Namrata Roy verfasserin aut Celia R. Mulcahey verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 945(2023), 2, p 117 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:945 year:2023 number:2, p 117 https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/article/68a54c123198430287c00f66c141e47a kostenfrei https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/toc/1538-4357 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_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 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 945 2023 2, p 117
allfieldsGer	10.3847/1538-4357/acba06 doi (DE-627)DOAJ089152085 (DE-599)DOAJ68a54c123198430287c00f66c141e47a DE-627 ger DE-627 rakwb eng QB460-466 Abdurro’uf verfasserin aut Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time? 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures. Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching Astrophysics Dan Coe verfasserin aut Intae Jung verfasserin aut Henry C. Ferguson verfasserin aut Gabriel Brammer verfasserin aut Kartheik G. Iyer verfasserin aut Larry D. Bradley verfasserin aut Pratika Dayal verfasserin aut Rogier A. Windhorst verfasserin aut Adi Zitrin verfasserin aut Ashish Kumar Meena verfasserin aut Masamune Oguri verfasserin aut Jose M. Diego verfasserin aut Vasily Kokorev verfasserin aut Paola Dimauro verfasserin aut Angela Adamo verfasserin aut Christopher J. Conselice verfasserin aut Brian Welch verfasserin aut Eros Vanzella verfasserin aut Tiger Yu-Yang Hsiao verfasserin aut Xinfeng Xu verfasserin aut Namrata Roy verfasserin aut Celia R. Mulcahey verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 945(2023), 2, p 117 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:945 year:2023 number:2, p 117 https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/article/68a54c123198430287c00f66c141e47a kostenfrei https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/toc/1538-4357 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_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 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 945 2023 2, p 117
allfieldsSound	10.3847/1538-4357/acba06 doi (DE-627)DOAJ089152085 (DE-599)DOAJ68a54c123198430287c00f66c141e47a DE-627 ger DE-627 rakwb eng QB460-466 Abdurro’uf verfasserin aut Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time? 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures. Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching Astrophysics Dan Coe verfasserin aut Intae Jung verfasserin aut Henry C. Ferguson verfasserin aut Gabriel Brammer verfasserin aut Kartheik G. Iyer verfasserin aut Larry D. Bradley verfasserin aut Pratika Dayal verfasserin aut Rogier A. Windhorst verfasserin aut Adi Zitrin verfasserin aut Ashish Kumar Meena verfasserin aut Masamune Oguri verfasserin aut Jose M. Diego verfasserin aut Vasily Kokorev verfasserin aut Paola Dimauro verfasserin aut Angela Adamo verfasserin aut Christopher J. Conselice verfasserin aut Brian Welch verfasserin aut Eros Vanzella verfasserin aut Tiger Yu-Yang Hsiao verfasserin aut Xinfeng Xu verfasserin aut Namrata Roy verfasserin aut Celia R. Mulcahey verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 945(2023), 2, p 117 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:945 year:2023 number:2, p 117 https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/article/68a54c123198430287c00f66c141e47a kostenfrei https://doi.org/10.3847/1538-4357/acba06 kostenfrei https://doaj.org/toc/1538-4357 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_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 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 945 2023 2, p 117
language	English
source	In The Astrophysical Journal 945(2023), 2, p 117 volume:945 year:2023 number:2, p 117
sourceStr	In The Astrophysical Journal 945(2023), 2, p 117 volume:945 year:2023 number:2, p 117
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching Astrophysics
isfreeaccess_bool	true
container_title	The Astrophysical Journal
authorswithroles_txt_mv	Abdurro’uf @@aut@@ Dan Coe @@aut@@ Intae Jung @@aut@@ Henry C. Ferguson @@aut@@ Gabriel Brammer @@aut@@ Kartheik G. Iyer @@aut@@ Larry D. Bradley @@aut@@ Pratika Dayal @@aut@@ Rogier A. Windhorst @@aut@@ Adi Zitrin @@aut@@ Ashish Kumar Meena @@aut@@ Masamune Oguri @@aut@@ Jose M. Diego @@aut@@ Vasily Kokorev @@aut@@ Paola Dimauro @@aut@@ Angela Adamo @@aut@@ Christopher J. Conselice @@aut@@ Brian Welch @@aut@@ Eros Vanzella @@aut@@ Tiger Yu-Yang Hsiao @@aut@@ Xinfeng Xu @@aut@@ Namrata Roy @@aut@@ Celia R. Mulcahey @@aut@@
publishDateDaySort_date	2023-01-01T00:00:00Z
hierarchy_top_id	269019219
id	DOAJ089152085
language_de	englisch
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callnumber-first	Q - Science
author	Abdurro’uf
spellingShingle	Abdurro’uf misc QB460-466 misc Galaxy evolution misc Galaxy formation misc Galaxy clusters misc Galaxy quenching misc Astrophysics Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?
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topic_title	QB460-466 Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time? Galaxy evolution Galaxy formation Galaxy clusters Galaxy quenching
topic	misc QB460-466 misc Galaxy evolution misc Galaxy formation misc Galaxy clusters misc Galaxy quenching misc Astrophysics
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title	Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?
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title_full	Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?
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author_browse	Abdurro’uf Dan Coe Intae Jung Henry C. Ferguson Gabriel Brammer Kartheik G. Iyer Larry D. Bradley Pratika Dayal Rogier A. Windhorst Adi Zitrin Ashish Kumar Meena Masamune Oguri Jose M. Diego Vasily Kokorev Paola Dimauro Angela Adamo Christopher J. Conselice Brian Welch Eros Vanzella Tiger Yu-Yang Hsiao Xinfeng Xu Namrata Roy Celia R. Mulcahey
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title_sort	spatially resolved stellar populations of 0.3 < z < 6.0 galaxies in whl 0137–08 and macs 0647+70 clusters as revealed by jwst: how do galaxies grow and quench over cosmic time?
callnumber	QB460-466
title_auth	Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?
abstract	We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures.
abstractGer	We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures.
abstract_unstemmed	We study the spatially resolved stellar populations of 444 galaxies at 0.3 < z < 6.0 in two clusters (WHL 0137–08 and MACS 0647+70) and a blank field, combining imaging data from the Hubble Space Telescope and JWST to perform spatially resolved spectral energy distribution (SED) modeling using piXedfit . The high spatial resolution of the imaging data combined with magnification from gravitational lensing in the cluster fields allows us to resolve a large fraction of our galaxies (109) to subkiloparsec scales. At redshifts around cosmic noon and higher (2.5 ≲ z ≲ 6.0), we find mass-doubling times to be independent of radius, inferred from flat specific star formation rate (sSFR) radial profiles and similarities between the half-mass and half-SFR radii. At lower redshifts (1.5 ≲ z ≲ 2.5), a significant fraction of our star-forming galaxies shows evidence for nuclear starbursts, inferred from a centrally elevated sSFR and a much smaller half-SFR radius compared to the half-mass radius. At later epochs, we find more galaxies suppress star formation in their centers but are still actively forming stars in the disk. Overall, these trends point toward a picture of inside-out galaxy growth consistent with theoretical models and simulations. We also observe a tight relationship between the central mass surface density and global stellar mass with ∼0.38 dex scatter. Our analysis demonstrates the potential of spatially resolved SED analysis with JWST data. Future analysis with larger samples will be able to further explore the assembly of galaxy mass and the growth of their structures.
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container_issue	2, p 117
title_short	Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?
url	https://doi.org/10.3847/1538-4357/acba06 https://doaj.org/article/68a54c123198430287c00f66c141e47a https://doaj.org/toc/1538-4357
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Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137–08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?

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