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- W4310184863 abstract "Abstract The Hawaii Survey Field SSA22 is the fourth deepest Chandra X-ray field. To allow for the fullest exploration of this field, we present new optical spectroscopy from Keck/DEIMOS and Keck/LRIS, which, in combination with the literature, brings the spectroscopic completeness of the 2–8 keV sample to 62%. We also make optical spectral classifications and estimate photometric redshifts for the sources without spectroscopic redshifts. We then determine hard X-ray luminosity functions (XLFs) for the full sample of active galactic nuclei (AGNs), as well as for the broad-line AGNs (BLAGNs) and the non-BLAGNs separately. Our XLF for the full sample is in good agreement with the literature, showing relatively strong evolution over the redshift range 0.25 ≤ z < 4. The XLFs for the BLAGNs and the non-BLAGNs imply distinct evolution with redshift, with BLAGNs becoming increasingly dominant at higher redshifts and X-ray luminosities." @default.
- W4310184863 created "2022-11-30" @default.
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- W4310184863 date "2022-11-28" @default.
- W4310184863 modified "2023-10-14" @default.
- W4310184863 title "X-Ray Sources in the SSA22 Chandra Field" @default.
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- W4310184863 doi "https://doi.org/10.3847/1538-4357/ac9bfe" @default.
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