Table 2
Measured properties of faint AGNs in our sample.
Name | ![]() |
fesc (LyC) | S/N | M1450 |
---|---|---|---|---|
SDSS36 | 4.047 | 0.81 | 87 | –25.14 |
SDSS32 | 3.964 | 0.86 | 33 | –25.13 |
COSMOS775 | 3.609 | 0.74 | 31 | –24.14 |
SDSS37 | 4.173 | 1.00 | 121 | –24.94 |
NDWFSJ05 | 3.900 | 0.44 | 12 | –24.03 |
SDSS04 | 3.768 | 0.73 | 96 | –24.39 |
COSMOS1782 | 3.748 | 0.78 | 72 | –23.26 |
SDSS20 | 3.899 | 0.53 | 58 | –24.71 |
SDSS27 | 3.604 | 1.00 | 42 | –24.22 |
COSMOS955 | 3.715 | 0.51 | 84 | –24.65 |
COSMOS1311 | 3.736 | 0.51 | 29 | –24.53 |
SDSS3777 | 3.723 | 0.61 | 26 | –24.62 |
SDSS3793 | 3.743 | 0.84 | 12 | –24.51 |
SDSS3785 | 3.769 | 0.88 | 20 | –24.63 |
SDSS3832 | 3.663 | 0.88 | 11 | –24.72 |
UDS10275 | 4.096 | 0.75 | 27 | –23.80 |
MEAN | 3.82 | 0.74 | –24.46 |
Notes. The LyC escape fraction fesc (LyC) and the absolute magnitude M1450 were derived adopting the refined spectroscopic redshift . The S/N refers to the total flux in the LyC region, integrated between 892 and 905 Å rest frame. The errors on fesc (LyC) vary from ~2 to 15%, according to the measured S/N.
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