Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View

We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, incl...
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Autor*in:	Luca Costantin [verfasserIn] Pablo G. Pérez-González [verfasserIn] Jesús Vega-Ferrero [verfasserIn] Marc Huertas-Company [verfasserIn] Laura Bisigello [verfasserIn] Fernando Buitrago [verfasserIn] Micaela B. Bagley [verfasserIn] Nikko J. Cleri [verfasserIn] Michael C. Cooper [verfasserIn] Steven L. Finkelstein [verfasserIn] Benne W. Holwerda [verfasserIn] Jeyhan S. Kartaltepe [verfasserIn] Anton M. Koekemoer [verfasserIn] Dylan Nelson [verfasserIn] Casey Papovich [verfasserIn] Annalisa Pillepich [verfasserIn] Nor Pirzkal [verfasserIn] Sandro Tacchella [verfasserIn] L. Y. Aaron Yung [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 946(2023), 2, p 71
Übergeordnetes Werk:	volume:946 ; year:2023 ; number:2, p 71

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/acb926

Katalog-ID:	DOAJ088835367

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allfields	10.3847/1538-4357/acb926 doi (DE-627)DOAJ088835367 (DE-599)DOAJ923913397fe84f8fbc5eea6098c898a2 DE-627 ger DE-627 rakwb eng QB460-466 Luca Costantin verfasserin aut Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22 Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems Astrophysics Pablo G. Pérez-González verfasserin aut Jesús Vega-Ferrero verfasserin aut Marc Huertas-Company verfasserin aut Laura Bisigello verfasserin aut Fernando Buitrago verfasserin aut Micaela B. Bagley verfasserin aut Nikko J. Cleri verfasserin aut Michael C. Cooper verfasserin aut Steven L. Finkelstein verfasserin aut Benne W. Holwerda verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Anton M. Koekemoer verfasserin aut Dylan Nelson verfasserin aut Casey Papovich verfasserin aut Annalisa Pillepich verfasserin aut Nor Pirzkal verfasserin aut Sandro Tacchella verfasserin aut L. Y. Aaron Yung verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 946(2023), 2, p 71 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:946 year:2023 number:2, p 71 https://doi.org/10.3847/1538-4357/acb926 kostenfrei https://doaj.org/article/923913397fe84f8fbc5eea6098c898a2 kostenfrei https://doi.org/10.3847/1538-4357/acb926 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 946 2023 2, p 71
spelling	10.3847/1538-4357/acb926 doi (DE-627)DOAJ088835367 (DE-599)DOAJ923913397fe84f8fbc5eea6098c898a2 DE-627 ger DE-627 rakwb eng QB460-466 Luca Costantin verfasserin aut Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22 Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems Astrophysics Pablo G. Pérez-González verfasserin aut Jesús Vega-Ferrero verfasserin aut Marc Huertas-Company verfasserin aut Laura Bisigello verfasserin aut Fernando Buitrago verfasserin aut Micaela B. Bagley verfasserin aut Nikko J. Cleri verfasserin aut Michael C. Cooper verfasserin aut Steven L. Finkelstein verfasserin aut Benne W. Holwerda verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Anton M. Koekemoer verfasserin aut Dylan Nelson verfasserin aut Casey Papovich verfasserin aut Annalisa Pillepich verfasserin aut Nor Pirzkal verfasserin aut Sandro Tacchella verfasserin aut L. Y. Aaron Yung verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 946(2023), 2, p 71 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:946 year:2023 number:2, p 71 https://doi.org/10.3847/1538-4357/acb926 kostenfrei https://doaj.org/article/923913397fe84f8fbc5eea6098c898a2 kostenfrei https://doi.org/10.3847/1538-4357/acb926 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 946 2023 2, p 71
allfields_unstemmed	10.3847/1538-4357/acb926 doi (DE-627)DOAJ088835367 (DE-599)DOAJ923913397fe84f8fbc5eea6098c898a2 DE-627 ger DE-627 rakwb eng QB460-466 Luca Costantin verfasserin aut Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22 Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems Astrophysics Pablo G. Pérez-González verfasserin aut Jesús Vega-Ferrero verfasserin aut Marc Huertas-Company verfasserin aut Laura Bisigello verfasserin aut Fernando Buitrago verfasserin aut Micaela B. Bagley verfasserin aut Nikko J. Cleri verfasserin aut Michael C. Cooper verfasserin aut Steven L. Finkelstein verfasserin aut Benne W. Holwerda verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Anton M. Koekemoer verfasserin aut Dylan Nelson verfasserin aut Casey Papovich verfasserin aut Annalisa Pillepich verfasserin aut Nor Pirzkal verfasserin aut Sandro Tacchella verfasserin aut L. Y. Aaron Yung verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 946(2023), 2, p 71 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:946 year:2023 number:2, p 71 https://doi.org/10.3847/1538-4357/acb926 kostenfrei https://doaj.org/article/923913397fe84f8fbc5eea6098c898a2 kostenfrei https://doi.org/10.3847/1538-4357/acb926 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 946 2023 2, p 71
allfieldsGer	10.3847/1538-4357/acb926 doi (DE-627)DOAJ088835367 (DE-599)DOAJ923913397fe84f8fbc5eea6098c898a2 DE-627 ger DE-627 rakwb eng QB460-466 Luca Costantin verfasserin aut Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22 Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems Astrophysics Pablo G. Pérez-González verfasserin aut Jesús Vega-Ferrero verfasserin aut Marc Huertas-Company verfasserin aut Laura Bisigello verfasserin aut Fernando Buitrago verfasserin aut Micaela B. Bagley verfasserin aut Nikko J. Cleri verfasserin aut Michael C. Cooper verfasserin aut Steven L. Finkelstein verfasserin aut Benne W. Holwerda verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Anton M. Koekemoer verfasserin aut Dylan Nelson verfasserin aut Casey Papovich verfasserin aut Annalisa Pillepich verfasserin aut Nor Pirzkal verfasserin aut Sandro Tacchella verfasserin aut L. Y. Aaron Yung verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 946(2023), 2, p 71 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:946 year:2023 number:2, p 71 https://doi.org/10.3847/1538-4357/acb926 kostenfrei https://doaj.org/article/923913397fe84f8fbc5eea6098c898a2 kostenfrei https://doi.org/10.3847/1538-4357/acb926 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 946 2023 2, p 71
allfieldsSound	10.3847/1538-4357/acb926 doi (DE-627)DOAJ088835367 (DE-599)DOAJ923913397fe84f8fbc5eea6098c898a2 DE-627 ger DE-627 rakwb eng QB460-466 Luca Costantin verfasserin aut Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22 Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems Astrophysics Pablo G. Pérez-González verfasserin aut Jesús Vega-Ferrero verfasserin aut Marc Huertas-Company verfasserin aut Laura Bisigello verfasserin aut Fernando Buitrago verfasserin aut Micaela B. Bagley verfasserin aut Nikko J. Cleri verfasserin aut Michael C. Cooper verfasserin aut Steven L. Finkelstein verfasserin aut Benne W. Holwerda verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Anton M. Koekemoer verfasserin aut Dylan Nelson verfasserin aut Casey Papovich verfasserin aut Annalisa Pillepich verfasserin aut Nor Pirzkal verfasserin aut Sandro Tacchella verfasserin aut L. Y. Aaron Yung verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 946(2023), 2, p 71 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:946 year:2023 number:2, p 71 https://doi.org/10.3847/1538-4357/acb926 kostenfrei https://doaj.org/article/923913397fe84f8fbc5eea6098c898a2 kostenfrei https://doi.org/10.3847/1538-4357/acb926 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 946 2023 2, p 71
language	English
source	In The Astrophysical Journal 946(2023), 2, p 71 volume:946 year:2023 number:2, p 71
sourceStr	In The Astrophysical Journal 946(2023), 2, p 71 volume:946 year:2023 number:2, p 71
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems Astrophysics
isfreeaccess_bool	true
container_title	The Astrophysical Journal
authorswithroles_txt_mv	Luca Costantin @@aut@@ Pablo G. Pérez-González @@aut@@ Jesús Vega-Ferrero @@aut@@ Marc Huertas-Company @@aut@@ Laura Bisigello @@aut@@ Fernando Buitrago @@aut@@ Micaela B. Bagley @@aut@@ Nikko J. Cleri @@aut@@ Michael C. Cooper @@aut@@ Steven L. Finkelstein @@aut@@ Benne W. Holwerda @@aut@@ Jeyhan S. Kartaltepe @@aut@@ Anton M. Koekemoer @@aut@@ Dylan Nelson @@aut@@ Casey Papovich @@aut@@ Annalisa Pillepich @@aut@@ Nor Pirzkal @@aut@@ Sandro Tacchella @@aut@@ L. Y. Aaron Yung @@aut@@
publishDateDaySort_date	2023-01-01T00:00:00Z
hierarchy_top_id	269019219
id	DOAJ088835367
language_de	englisch
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callnumber-first	Q - Science
author	Luca Costantin
spellingShingle	Luca Costantin misc QB460-466 misc Galaxies misc Galactic and extragalactic astronomy misc High-redshift galaxies misc Late-type galaxies misc Irregular galaxies misc Galaxy classification systems misc Astrophysics Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
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topic_title	QB460-466 Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View Galaxies Galactic and extragalactic astronomy High-redshift galaxies Late-type galaxies Irregular galaxies Galaxy classification systems
topic	misc QB460-466 misc Galaxies misc Galactic and extragalactic astronomy misc High-redshift galaxies misc Late-type galaxies misc Irregular galaxies misc Galaxy classification systems misc Astrophysics
topic_unstemmed	misc QB460-466 misc Galaxies misc Galactic and extragalactic astronomy misc High-redshift galaxies misc Late-type galaxies misc Irregular galaxies misc Galaxy classification systems misc Astrophysics
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title	Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
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title_full	Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
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author_browse	Luca Costantin Pablo G. Pérez-González Jesús Vega-Ferrero Marc Huertas-Company Laura Bisigello Fernando Buitrago Micaela B. Bagley Nikko J. Cleri Michael C. Cooper Steven L. Finkelstein Benne W. Holwerda Jeyhan S. Kartaltepe Anton M. Koekemoer Dylan Nelson Casey Papovich Annalisa Pillepich Nor Pirzkal Sandro Tacchella L. Y. Aaron Yung
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title_sort	expectations of the size evolution of massive galaxies at 3 ≤ z ≤ 6 from the tng50 simulation: the ceers/jwst view
callnumber	QB460-466
title_auth	Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
abstract	We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22
abstractGer	We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22
abstract_unstemmed	We present a catalog of about 25,000 images of massive ( M _⋆ ≥ 10 ^9 M _⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST. The synthetic images were created with the SKIRT radiative transfer code, including the effects of dust attenuation and scattering. The noiseless images were processed with the mirage simulator to mimic the Near Infrared Camera (NIRCam) observational strategy (e.g., noise, dithering pattern, etc.) of the Cosmic Evolution Early Release Science (CEERS) survey. In this paper, we analyse the predictions of the TNG50 simulation for the size evolution of galaxies at 3 ≤ z ≤ 6 and the expectations for CEERS to probe that evolution. In particular, we investigate how sizes depend on the wavelength, redshift, mass, and angular resolution of the images. We find that the effective radius accurately describes the three-dimensional half-mass–radius of the TNG50 galaxies. Sizes observed at 2 μ m are consistent with those measured at 3.56 μ m at all redshifts and masses. At all masses, the population of higher- z galaxies is more compact than their lower- z counterparts. However, the intrinsic sizes are smaller than the mock observed sizes for the most massive galaxies, especially at z ≲ 4. This discrepancy between the mass and light distributions may point to a transition in the galaxy morphology at z = 4–5, where massive compact systems start to develop more extended stellar structures. ^22
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title_short	Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
url	https://doi.org/10.3847/1538-4357/acb926 https://doaj.org/article/923913397fe84f8fbc5eea6098c898a2 https://doaj.org/toc/1538-4357
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Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View

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