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- W2955442607 abstract "The exact formation mechanism of massive galaxy in the universe still become an open question in modern astrophysics. Radio emission from active galactic nucleus (AGN) is known to be suppressing stellar growth in the most massive galaxies, thus becoming significant ingredient in modeling galaxy formation process. Radio luminosity function across cosmic redshifts (z) is an important tool to constrain the co-evolutionary models of radio AGN and its host galaxy. Therefore, we aim to calculate radio luminosity function at 1.4 GHz frequency for radio AGN in the range of 0.1 ≤ z ≤ 1.3 in this work. The radio data was taken from deep VLA observation of Stripe 82 field at angular resolution of 1.8 and 52 μJy sensitivity. On the other hand, the optical/near-infrared data was taken from Dark Energy Survey DR1 observation in g, r, i, z, Y bands with co-added catalog limiting magnitude of i = 23.44." @default.
- W2955442607 created "2019-07-12" @default.
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- W2955442607 date "2019-05-01" @default.
- W2955442607 modified "2023-09-27" @default.
- W2955442607 title "Cosmic Evolution of Nearby Radio Active Galactic Nuclei" @default.
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- W2955442607 doi "https://doi.org/10.1088/1742-6596/1231/1/012005" @default.
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