An AGN is an active galactic nucleus, a compact region at the centre of a galaxy with a much higher than normal luminosity over some portion, possibly all, of the electromagnetic spectrum.
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An AGN is an active galactic nucleus, a compact region at the centre of a galaxy with a much higher than normal luminosity over some portion, possibly all, of the electromagnetic spectrum.
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Yes, an AGN is a compact region at the center of a galaxy that has a much higher than normal luminosity, over at least some portion, and possibly all, of the electromagnetic spectrum.
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The possible error of an Active Galactic Nucleus (AGN) photometry (AGP) can arise from various factors, including calibration uncertainties, intrinsic variability of the AGN, and atmospheric conditions affecting observations. Additionally, errors may stem from the choice of the model used for fitting the light curves and the methods employed for background subtraction. These factors can lead to discrepancies in the measured brightness, spectral properties, and overall interpretation of AGN behavior. Proper statistical analysis and error estimation techniques are essential for mitigating these potential inaccuracies.
The energy emitted by AGN and quasars most likely originates from the supermassive black hole at their center. As matter falls into the black hole, it releases energy in the form of radiation and powerful jets of particles, creating the intense emission observed from these objects.