A New Record Census of Dwarf AGN and a Bimodal $M_{\mathrm{BH}}$-$M_{\star }$ Scaling Relation with DESI DR1

Abstract

Using the first spectroscopic data release from the Dark Energy Spectroscopic Instrument (DESI DR1), we search for AGN signatures in 1,678,787 low-redshift ($0.001\le z\le 0.45$) line-emitting galaxies. Based on the [NII]-BPT emission-line ratio diagnostic, we identify AGN in 314,245/1,211,573 (25.9%) high-mass ($\log (M_{\star }/M_{\odot })>9.5$) and 9648/467,214 (2.1%) dwarf ($\log (M_{\star }/M_{\odot })\le 9.5$) galaxies. Among these AGN, 17,949 are broad-line candidates (BL-AGN) with broad H$\hat{I}\pm$ emission, enabling black hole (BH) mass estimates using single-epoch virial methods. We find that the AGN fraction in line-emitting galaxies increases monotonically with stellar mass, rising from $\sim$1.4% at the low-mass end to $\sim$93.3% at the high-mass end. Using the large BL-AGN sample, we extend the $M_{\mathrm{BH}}-M_{\star }$ scaling relation down to $\log (M_{\star }/M_{\odot })\approx 7.8$ and $\log (M_{\mathrm{BH}}/M_{\odot })\approx 4.4$. In the context of high-redshift overmassive BHs, our results suggest that galaxies and their central BHs may follow two distinct evolutionary pathways across cosmic time. With this paper, we release the EmFit value-added catalog, containing emission-line flux and width measurements for $\sim$7.4 million galaxies, the largest catalog with emission-line decomposition into narrow, broad, and outflow components to date. This work significantly expands upon the early DESI results and provides a statistical sample for probing the galaxy$-$BH connection in the low-mass galaxy regime.

32 pages, 15 figures, Submitted to AAS Journals