Metallicity in Quasar Broad Line Regions at Redshift 6
arXiv:2112.07799 · doi:10.3847/1538-4357/ac3a69
Abstract
Broad line regions (BLRs) in high-redshift quasars provide crucial information of chemical enrichment in the early universe. Here we present a study of BLR metallicities in 33 quasars at redshift . Using the near-IR spectra of the quasars obtained from the Gemini telescope, we measure their rest-frame UV emission line flux and calculate flux ratios. We then estimate BLR metallicities with empirical calibrations based on photoionization models. The inferred median metallicity of our sample is a few times the solar value, indicating that the BLR gas had been highly metal-enriched at . We compare our sample with a low-redshift quasar sample with similar luminosities and find no evidence of redshift evolution in quasar BLR metallicities. This is consistent with previous studies. The Fe IIMg II flux ratio, a proxy for the Fe element abundance ratio, shows no redshift evolution as well, further supporting rapid nuclear star formation at . We also find that the black hole mass-BLR metallicity relation at is consistent with the relation measured at , suggesting that our results are not biased by a selection effect due to this relation.
ApJ, in press
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