The Astrophysical Journal (Jan 2024)

A SPectroscopic Survey of Biased Halos In the Reionization Era (ASPIRE): Broad-line AGN at z = 4−5 Revealed by JWST/NIRCam WFSS

  • Xiaojing Lin,
  • Feige Wang,
  • Xiaohui Fan,
  • Zheng Cai,
  • Jaclyn B. Champagne,
  • Fengwu Sun,
  • Marta Volonteri,
  • Jinyi Yang,
  • Joseph F. Hennawi,
  • Eduardo Bañados,
  • Aaron Barth,
  • Anna-Christina Eilers,
  • Emanuele Paolo Farina,
  • Weizhe Liu,
  • Xiangyu Jin,
  • Hyunsung D. Jun,
  • Alessandro Lupi,
  • Koki Kakiichi,
  • Chiara Mazzucchelli,
  • Masafusa Onoue,
  • Zhiwei Pan,
  • Elia Pizzati,
  • Sofía Rojas-Ruiz,
  • Jan-Torge Schindler,
  • Benny Trakhtenbrot,
  • Yue Shen,
  • Maxime Trebitsch,
  • Ming-Yang Zhuang,
  • Ryan Endsley,
  • Romain A. Meyer,
  • Zihao Li,
  • Mingyu Li,
  • Maria Pudoka,
  • Wei Leong Tee,
  • Yunjing Wu,
  • Haowen Zhang

DOI
https://doi.org/10.3847/1538-4357/ad6565
Journal volume & issue
Vol. 974, no. 1
p. 147

Abstract

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Low-luminosity active galactic nuclei (AGNs) with low-mass black holes (BHs) in the early universe are fundamental to understanding the BH growth and their coevolution with the host galaxies. Utilizing JWST NIRCam Wide Field Slitless Spectroscopy, we perform a systematic search for broad-line H α emitters (BHAEs) at z ≈ 4–5 in 25 fields of the A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE) project, covering a total area of 275 arcmin ^2 . We identify 16 BHAEs with FWHM of the broad components spanning from ∼1000 to 3000 km s ^−1 . Assuming that the broad line widths arise as a result of Doppler broadening around BHs, the implied BH masses range from 10 ^7 to 10 ^8 M _⊙ , with broad H α -converted bolometric luminosities of 10 ^44.5 –10 ^45.5 erg s ^−1 and Eddington ratios of 0.07–0.47. The spatially extended structure of the F200W stacked image may trace the stellar light from the host galaxies. The H α luminosity function indicates an increasing AGN fraction toward the higher H α 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 H α emitters. Three BHAEs exhibit blueshifted absorption troughs indicative of the presence of high column density gas. We find that the broad-line-selected 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 H α sample provides a good database for future studies of faint AGN populations at high redshift.

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