JADES: Differing assembly histories of galaxies
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Abstract
We used deep NIRSpec spectroscopic data from the JADES survey to derive the star formation histories (SFHs) of a sample of 200 galaxies at 0.6 < z < 11 that span stellar masses from 10 6 to 10 9.5 M ⊙ . We found that galaxies at high redshift, galaxies above the main sequence (MS), and low-mass galaxies tend to host younger stellar populations than their lower-redshift, below the MS, and more massive counterparts. Interestingly, the correlation between age, stellar mass M * , and star formation rate (SFR) existed even earlier than cosmic noon, out to the earliest cosmic epochs. However, these trends have a large scatter. There are also examples of young stellar populations below the MS, which indicates…
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Authors
35Topics & keywords
Topics
Keywords
- Physics
- Astrophysics
- Galaxy
- Redshift
- Star formation
- Stellar mass
- Billion years
- COSMIC cancer database
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Funding
- NSNational Science Foundation
- URUK Research and InnovationAwards: 101040227, PID2021-127718NB-I00
- ECEuropean CommissionAwards: ST/W001438/1, 789056, 10.13039/501100011033, MICIN/AEI/10.13039/501100011033, 13039/501100011033, 501100011033, 695671, 101040227, AEI/10.13039/501100011033
- NRNational Research Foundation
- DGDanmarks Grundforskningsfond
- INIsaac Newton Trust
- MDMinisterio de Ciencia e InnovaciónAwards: AEI/ 10.13039/501100011033, 10.13039, AEI/10.13039/501100011033, PID2021-127718NB-I00, 501100011033, AEI/10, 10.13039/501100011033, 13039/501100011033, MICIN/AEI/ 10.13039/501100011033, MICIN/AEI/10.13039/501100011033, /AEI/10.13039/501100011033
- FMFondation Merac
- SAScience and Technology Facilities CouncilAwards: ST/W001438/1, PID2021-127718NB-I00, /10.13039/501100011033, NAS5-02015, CE170100013, ST/S004831/1, 695671
- EREuropean Research Council
- AEAgencia Estatal de InvestigaciónAwards: AEI/10.13039/501100011033, 501100011033, 10.13039/501100011033, AEI/ 10.13039/501100011033, 13039, 10.13039, AEI/10, 13039/501100011033, AEI/10., MICIN/AEI/10.13039/501100011033