The Star-forming Main Sequence and Bursty Star-formation Histories at $z>1.4$ in JADES and AURORA

Abstract

We analyze JWST spectroscopic and HST+JWST photometric observations of 659 star-forming galaxies at $1.4<z<9$ from DR3 of the JADES survey and the AURORA Cycle 1 program. We measure the star-forming main sequence (SFMS) for galaxies above $10^{8.5}\rm\ M_\odot$ where the sample is largely representative, estimating star-formation rates (SFRs) using the H$\alpha$ line flux and rest-frame far UV (1600\AA) continuum measurements, each independently corrected for dust attenuation. We find that the intrinsic, measurement-error-subtracted scatter in the SFMS ($\sigma_{\rm int}$) increases with decreasing stellar mass for the H$\alpha$-based SFMS, and we find no mass dependence of $\sigma_{\rm int}$ in the UV-based SFMS. Additionally, we find that $\sigma_{\rm int}$ decreases with increasing redshift, from $0.36^{+0.02}_{-0.02}$ dex to $0.22^{+0.08}_{-0.07}$ dex (H$\alpha$ SFMS), and from $0.28^{+0.02}_{-0.02}$ dex to $0.20^{+0.08}_{-0.07}$ dex (UV SFMS) between $z\sim2$ and $z\sim 6.5$. We also measure the redshift evolution of the specific SFR and find that, assuming $\rm sSFR\propto (1+z)^\gamma$, $\gamma=1.89^{+0.16}_{-0.15}$ for the H$\alpha$-based SFMS, and $\gamma=1.36^{+0.13}_{-0.13}$ for the UV-based SFMS. Analyzing the observed H$\alpha$/UV luminosity ratios and star-formation histories from the {\sc prospector} fitting code, we find that 41--60\% of the sample is inconsistent with having a constant star-formation history. Finally, we find tentative evidence for shorter SFR burst timescales with increasing redshift based on the distribution of $\rm L_{H\alpha}/\nu L_{\nu,1600}$ vs. $\Delta\rm \log(L_{H\alpha})$. Taken together, these results are consistent with recent theoretical predictions (e.g., the {\sc thesan-zoom} simulations) of bursty star formation in the early Universe and provide valuable constraints for theoretical models of galaxy evolution.