ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-ray Detected Active Galactic Nuclei

Abstract

We report the multi-wavelength properties of millimeter galaxies hosting X-ray detected active galactic nuclei (AGNs) from the ALMA Lensing Cluster Survey (ALCS). ALCS is an extensive survey of well-studied lensing clusters with ALMA, covering an area of 133 arcmin${}^2$ over 33 clusters with a 1.2 mm flux-density limit of $\sim$60 $\mu \mathrm{Jy}$ ($1\sigma$). Utilizing the archival data of Chandra, we identify three AGNs at $z=$1.06, 2.09, and 2.84 among the 180 millimeter sources securely detected in the ALCS (of which 155 are inside the coverage of Chandra). The X-ray spectral analysis shows that two AGNs are not significantly absorbed ($\log N_{\mathrm{H}}/{\mathrm{cm}}^{-2}<23$), while the other shows signs of moderate absorption ($\log N_{\mathrm{H}}/{\mathrm{cm}}^{-2}\sim 23.5$). We also perform spectral energy distribution (SED) modelling of X-ray to millimeter photometry. We find that our X-ray AGN sample shows both high mass accretion rates (intrinsic 0.5--8 keV X-ray luminosities of $\sim 10^{\text{44–45}}\mathrm{erg}{\mathrm{s}}^{-1}$) and star-formation rates ($\gtrsim 100M_{\odot }{\mathrm{yr}}^{-1}$). This demonstrates that a wide-area survey with ALMA and Chandra can selectively detect intense growth of both galaxies and supermassive black holes (SMBHs) in the high-redshift universe.

arXiv comment14 pages, 3 figures, 2 tables

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