The Rise of Faint, Red AGN at z>4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields
arxiv(2024)
摘要
We present a sample of 341 "little red dots" (LRDs) spanning the redshift
range z∼2-11 using data from the CEERS, PRIMER, JADES, UNCOVER and NGDEEP
surveys. These sources are likely heavily-reddened AGN that trace a
previously-hidden phase of dust-obscured black hole growth in the early
Universe. Unlike past use of color indices to identify LRDs, we employ
continuum slope fitting using shifting bandpasses to sample the same rest-frame
emission blueward and redward of the Balmer break. This approach allows us to
identify LRDs over a wider redshift range and is less susceptible to
contamination from galaxies with strong breaks that otherwise lack a rising red
continuum. The redshift distribution of our sample increases at z<8 and then
undergoes a rapid decline at z∼4.5, which may tie the emergence, and
obscuration, of these sources to the inside-out growth that galaxies experience
during this epoch. We find that LRDs are 2-3 dex more numerous than bright
quasars at z∼5-7, but their number density is only 0.6-1 dex higher than
X-ray and UV selected AGN at these redshifts. Within our sample, we have
identified the first X-ray detected LRDs at z=3.1 and z=4.66. An X-ray
spectral analysis confirms that these AGN are moderately obscured with
log (N_ H/ cm^2) of 23.3^+0.4_-1.3 and
22.72^+0.13_-0.16. Our analysis reveals that reddened AGN emission
dominates their rest-optical light, while the rest-UV originates from their
host galaxies. We also present NIRSpec follow-up spectroscopy of 17 LRDs that
show broad emission lines consistent with AGN activity. The confirmed AGN
fraction of our sample is 71% for sources with F444W<26.5. In addition, we
find three LRDs with narrow blue-shifted Balmer absorption features in their
spectra, suggesting an outflow of high-density, low ionization gas from near
the central engine of these faint, red AGN.
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