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Bursting at the seams: the star-forming main sequence and its scatter at z = 3–9 using NIRCam photometry from JADES

Abstract:
We present a comprehensive study of the star-forming main sequence (SFMS) and its scatter at redshifts , using Near Infrared Camera (NIRCam) photometry from the JADES (JWST Advanced Deep Extragalactic Survey) survey in the Great Observatories Origins Deep Survey (GOODS) South (GOODS-S) and North (GOODS-N) fields. Our analysis is based on a sample of galaxies that is stellar mass complete down to . The redshift evolution of the SFMS at an averaging time-scale of 10 Myr follows a relation, quantified by the specific star formation rates (sSFR), of with , in good agreement with theoretical predictions and the specific mass accretion rate of dark matter haloes. We find that the SFMS normalization varies in a complex way with the SFR averaging time-scale, reflecting the combined effects of bursty star formation and rising star formation histories (SFHs). We quantify the scatter of the SFMS, revealing that it decreases with longer SFR averaging time-scales, from at 10 Myr to at 100 Myr, indicating that shorter term fluctuations dominate the scatter, although long-term variations in star formation activity are also present. Our findings suggest that bursty SFHs are more pronounced at lower stellar masses. Furthermore, we explore the implications of our results for the observed overabundance of UV-bright galaxies at , concluding that additional mechanisms, such as top-heavy initial mass functions, increased star formation efficiencies, or increased burstiness in star formation are needed to explain these observations. Finally, we emphasize the importance of accurate stellar mass completeness limits when fitting the SFMS, especially for galaxies with bursty SFHs.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/staf1950

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Author
ORCID:
0000-0003-4770-7516
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ORCID:
0000-0002-8224-4505
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Author
ORCID:
0009-0009-5565-3790
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Author
ORCID:
0000-0002-9551-0534


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Funder identifier:
https://ror.org/03m2x1q45
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https://ror.org/021nxhr62
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Funder identifier:
https://ror.org/00yjd3n13
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https://ror.org/03wd9za21


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
544
Issue:
4
Pages:
4551-4575
Publication date:
2025-11-06
Acceptance date:
2025-11-03
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
UUID:
uuid_2f36072d-db62-4ecd-9cc2-36719eebb3ee
Source identifiers:
3539636
Deposit date:
2025-12-05
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