paper

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Broad-line AGN at revealed by JWST/NIRCam WFSS

arXiv:2407.17570

Abstract

Low-luminosity AGNs with low-mass black holes (BHs) in the early universe are fundamental to understanding the BH growth and their co-evolution with the host galaxies. Utilizing JWST NIRCam Wide Field Slitless Spectroscopy (WFSS), we perform a systematic search for broad-line emitters (BHAEs) at in 25 fields of the ASPIRE (A SPectroscopic survey of biased halos In the Reionization Era) project, covering a total area of 275 arcmin. We identify 16 BHAEs with FWHM of the broad components spanning from 1000 km s to 3000 km s. Assuming the broad linewidths arise due to Doppler broadening around BHs, the implied BH masses range from to , with broad -converted bolometric luminosity of erg s and Eddington ratios of . The spatially extended structure of the F200W stacked image may trace the stellar light from the host galaxies. The luminosity function indicates an increasing AGN fraction towards the higher luminosities. We find possible evidence for clustering of BHAEs: two sources are at the same redshift with a projected separation of 519 kpc; one BHAE appears as a composite system residing in an overdense region with three close companion emitters. Three BHAEs exhibit blueshifted absorption troughs indicative of the presence of high-column-density gas. We find the broad-line and photometrically selected BHAE samples exhibit different distributions in the optical continuum slopes, which can be attributed to their different selection methods. The ASPIRE broad-line sample provides a good database for future studies of faint AGN populations at high redshift.

19 pages, 13 figures, 4 tables. Accepted by the ApJ

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Broad-line AGN at $z=4-5$ revealed by JWST/NIRCam WFSS · wovepaper